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RYU, CHANG MO (유창모)
Dept of Physics(물리학과)
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POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY 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SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA INTERACTION:1||GAS:1||Capacitivelycoupled plasma:1||Magnetic field:1||PULSE:1||ABSORPTION:1||HYDROMAGNETICWAVES:1||DECAY INSTABILITY:1||EVOLUTION:1||ATMOSPHERICPRESSURE:1||ICP:1||SOLAR RADIOBURSTS:1||particleincell simulation:1||RF DISCHARGE:1||GAUSSIAN APPROXIMATION:1||s function:1||PERSISTENT CURRENTS:1||CORONAL LOOPS:1||QUANTUM TRANSPORT:1||ELECTRONS:1||MASSIVE GAUGETHEORIES:1||WAVEGUIDES:1||plasma turbulence:1||FLUCTUATIONS:1||PARTICLE SIMULATIONS:1||NONLINEAR EVOLUTION:1||IONCYCLOTRON:1||BURSTS:1||SATURNS MAGNETOSPHERE:1||Tokamak plasmas:1||JET:1||Electromagnetic sideband waves:1||UNDERDENSE PLASMAS:1||MODULATIONAL INSTABILITY:1||SIMULATIONS:1||SMALL COLD BEAM:1||dualfrequency:1||magnetic field:1||coulomb blockade:1||SYSTEM:1||LEADS:1||IONCYCLOTRON FREQUENCY:1||zonal flow:1||HYBRID DRIFT INSTABILITY:1||CURRENT DISRUPTION:1||ENERGYSPECTRA:1||WAVES:1||PARAMETRICINSTABILITIES:1||DRIVEN:1||SPECTRUM:1||atmosphericpressure glow discharge (APGD):1||Eigenvalue equations:1||Harmonic modes:1||Lowfrequency:1||Shear flow:1||WIND:1||ION KINETICS:1||CORONA:1||DRIFTWAVE TURBULENCE:1||COUPLEDCLUSTER METHOD:1||BCS SUPERCONDUCTIVITY:1||STATISTICS:1||QUANTUM:1||OSCILLATIONS:1||ION ENERGYDISTRIBUTION:1||DYNAMOS:1||WAVE:1||mirror plasma:1||EARTHS MAGNETOTAIL:1||Plasma simulation:1||ELECTROMAGNETIC EMISSION:1||Generalized weak turbulence theory:1||microplasma:1||kinetic simulation:1||Eigenvalue solvers:1||Reversed shear:1||TOKAMAKS:1||Stimulated Raman forward scattering:1||NONSTANDARD EXPANSION TECHNIQUES:1||superconductivity:1||REGIME:1||FRACTIONAL STATISTICS:1||BALLISTICTRANSPORT:1||H/E:1||DOUBLELAYERS:1||REVERSED CONFIGURATIONS:1||DISCHARGES:1||dusty plasma:1||dust ion acoustic solitary wave:1||MAGNETIC NEUTRAL SHEET:1||KSTAR:1||PLASMA SHEET:1||PRESSURE RF DISCHARGE:1||microdischarge:1||DISCHARGE:1||Tokamak devices:1||Prelaser pulses:1||BEAM:1||ACCELERATION:1||Hanbit:1||TURBULENCE THEORY:1||RESONANCE:1||INTERFERENCE:1||ALLOYS:1||radiations in plasmas:1||HEATINGMODE TRANSITION:1||PINCH:1||beam plasma interaction:1||Langmuir turbulence:1||ANOMALOUS RESISTIVITY:1||III RADIOBURSTS:1||Raman instability:1||INTENSE LASER:1||Plasma emission:1||AMPLIFICATION:1||Dualfrequency:1||TRANSITION:1||PARTICLE:1||Magnetoplasma:1||POLYMERS:8||ADHESION:8||PLASMA:7||XPS:6||plasma:6||TRANSPORT:5||DYNAMICS:5||argon:4||FILMS:4||crosslinking:4||oxygen:4||SYSTEMS:4||crystallinity:4||MODEL:4||STATES:4||aging:4||MECHANISM:4||SPIN:3||TOKAMAK:3||GENERATION:3||MODES:3||THIN CURRENT SHEETS:3||LOOPS:3||SOLARWIND:3||GLOWDISCHARGE:3||SIMULATION:3||TURBULENCE:3||INSTABILITY:3||SPECTRA:3||STABILITY:2||HARMONIC LANGMUIRWAVES:2||TREATED SILICONERUBBER:2||HYDROPHOBIC RECOVERY:2||JUNCTIONS:2||CRITERION:2||SINGLE:2||STABILIZATION:2||Electron beamplasma instability:2||BOUNDARY:2||SPACE PLASMAS:2||MAGNETICFIELD:2||ELECTROMAGNETICRADIATION:2||SURFACE MODIFICATION:2||TIME:2||PRESSURE:2||BALLOONING INSTABILITY:2||TAIL:2||POLYPROPYLENE:2||SCATTERING:2||ENERGY:2||CONTACTANGLE:2||photonassisted tunneling:2||FLUX TUBES:2||NEUTRAL PARTICLES:2||INTERCHANGE MODES:2||AIR:2||EQUATIONS:2||PARTICLES:2||TWOFOLDDEGENERATE BAND:2||oxygenplasma:2||ABSORPTION SPECTROSCOPY NEXAFS:2||SURFACEANALYSIS:2||HDPE:2||SURFACE:2||angleresolved XPS:2||AMORPHOUS FERROMAGNETS:2||SOLAR ATMOSPHERE:2||highdensity polyethylene:2||surface rearrangement:2||SHEATH:2||CORONA DISCHARGE:2||WATER:2||ZONAL FLOWS:2||BICOHERENCE:2||SUBSTORM ONSET:2||LDPE:2||THERMOPOWER:2||FLOW:2||BERRY PHASE:2||SEARCH:2||PLASMA INSTABILITIES:2||TEMPERATURE:2||INTERPLANETARY SPACE:2||HIGHINTENSITY LASERS:1||FINITEAMPLITUDE:1||IONS:1||NONLINEARINTERACTION:1||ELECTRONBEAMS:1||QUANTUMFIELD THEORY:1||superconductor:1||quasiparticle transport:1||DISCRETE ELECTRONIC STATES:1||microwave:1||BEHAVIOR:1||FLUX:1||dwave superconductor:1||QUANTUMMECHANICS:1||energetic particle:1||STRANGE ATTRACTORS:1||PROFILE:1||CODE:1||STOCHASTIC ACCELERATION:1||Laserplasma interaction:1||Self focusing harmonic generation density ripple plasma:1||Particleincell simulation:1||Alfven eigenmodes:1||Eigenvalues and eigenfunctions:1||Critical value:1||EIGENMODES:1||EXCITATION:1||ELECTRON ACCELERATION:1||RFTF:1||capacitively coupled plasma:1||PERTURBATIVE EXPANSION:1||OPTIMIZED EXPANSION:1||SUPERCONDUCTIVITY:1||nonequilibrium Green&apos:1||quantum dot:1||SINGLEELECTRON TRANSISTOR:1||electrical resistivity:1||MESOSCOPIC RINGS:1||CURRENT MAGNIFICATION:1||RESONANTLY COUPLED CAVITIES:1||NORMALMETAL RINGS:1||VOLTAGE:1||KINK INSTABILITY:1||MAGNETOTAIL:1||DISRUPTION:1||DISPERSION FUNCTION:1||Cluster plasma:1||LASER:1||EMISSION:1||FREQUENCY:1||PLASMAS:1||HELIUM:1||KAPPADISTRIBUTIONS:1||CATHODEDISCHARGE:1||DEVICES:1||INSTABILITIES:1||LANGMUIRWAVES:1||RENORMALIZATION:1||tunneling current:1||PHASE:1||LOOP:1||TRANSMISSION:1||weak turbulence:1||RF DISCHARGES:1||RF FIELD:1||bispectral analysis:1||COHERENT:1||correlation dimension:1||edge turbulence:1||EARTHS MAGNETOSPHERE:1||Ideal MHD stability:1||BEAMPLASMA I
