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Cited 28 time in webofscience Cited 30 time in scopus
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dc.contributor.authorRyu, CM-
dc.contributor.authorTongnyeol Rhee-
dc.contributor.authorUmeda, T-
dc.contributor.authorPeter H. Yoon-
dc.contributor.authorOmura, Y-
dc.date.accessioned2015-06-25T03:21:23Z-
dc.date.available2015-06-25T03:21:23Z-
dc.date.created2010-04-30-
dc.date.issued2007-10-
dc.identifier.issn1070-664X-
dc.identifier.other2015-OAK-0000007271en_US
dc.identifier.urihttps://oasis.postech.ac.kr/handle/2014.oak/12593-
dc.description.abstractIn a recent paper it was suggested on the basis of weak turbulence theory that the collisionality of a plasma, coupled with nonlinear wave-particle interaction, is crucial for the acceleration of electrons by Langmuir turbulence to a superthermal energy level. In this Letter, fully nonlinear Vlasov and particle-in-cell (PIC) simulation techniques are employed to further verify this potentially important finding. The previous conclusion is fully confirmed by observing the expected difference between the Vlasov and PIC simulation results in the weak beam regime. However, in the strong beam regime, both the Vlasov and PIC simulations are found to produce a high-energy tail population, which indicates that there may be other mechanisms in the high beam speed situation, that are responsible for the generation the superthermal electrons. (C) 2007 American Institute of Physics.-
dc.description.statementofresponsibilityopenen_US
dc.languageEnglish-
dc.publisherAMER INST PHYSICS-
dc.relation.isPartOfPHYSICS OF PLASMAS-
dc.rightsBY_NC_NDen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/2.0/kren_US
dc.titleTurbulent acceleration of superthermal electrons-
dc.typeArticle-
dc.contributor.college물리학과en_US
dc.identifier.doi10.1063/1.2779282-
dc.author.googleRyu, CMen_US
dc.author.googleRhee, Ten_US
dc.author.googleOmura, Yen_US
dc.author.googleYoon, PHen_US
dc.author.googleUmeda, Ten_US
dc.relation.volume14en_US
dc.relation.issue10en_US
dc.relation.startpage100701-1en_US
dc.relation.lastpage100701-4en_US
dc.contributor.id10051262en_US
dc.relation.journalPHYSICS OF PLASMASen_US
dc.relation.indexSCI급, SCOPUS 등재논문en_US
dc.relation.sciSCIen_US
dc.collections.nameJournal Papersen_US
dc.type.rimsART-
dc.identifier.bibliographicCitationPHYSICS OF PLASMAS, v.14, no.10, pp.100701-1 - 100701-4-
dc.identifier.wosid000250589700001-
dc.date.tcdate2019-01-01-
dc.citation.endPage100701-4-
dc.citation.number10-
dc.citation.startPage100701-1-
dc.citation.titlePHYSICS OF PLASMAS-
dc.citation.volume14-
dc.contributor.affiliatedAuthorRyu, CM-
dc.identifier.scopusid2-s2.0-36048948062-
dc.description.journalClass1-
dc.description.journalClass1-
dc.description.wostc21-
dc.description.scptc21*
dc.date.scptcdate2018-10-274*
dc.type.docTypeArticle-
dc.subject.keywordPlusENERGY-SPECTRA-
dc.subject.keywordPlusDOUBLE-LAYERS-
dc.subject.keywordPlusPLASMA-
dc.subject.keywordPlusBEAM-
dc.subject.keywordPlusPARTICLES-
dc.subject.keywordPlusWAVES-
dc.subject.keywordPlusDISTRIBUTIONS-
dc.subject.keywordPlusGENERATION-
dc.subject.keywordPlusRADIATION-
dc.subject.keywordPlusCOMPONENT-
dc.relation.journalWebOfScienceCategoryPhysics, Fluids & Plasmas-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaPhysics-

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