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Cited 6 time in webofscience Cited 7 time in scopus
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dc.contributor.authorWoo, MH-
dc.contributor.authorRyu, CM-
dc.contributor.authorChoi, CR-
dc.date.accessioned2015-06-25T03:21:58Z-
dc.date.available2015-06-25T03:21:58Z-
dc.date.created2010-12-02-
dc.date.issued2010-05-
dc.identifier.issn1070-664X-
dc.identifier.other2015-OAK-0000022168en_US
dc.identifier.urihttps://oasis.postech.ac.kr/handle/2014.oak/12608-
dc.description.abstractAn obliquely propagating solitary kinetic Alfven wave in a low beta dusty plasma (beta << m(e)/m(i)) is studied by considering the ion motion along the magnetic field and the collisional effect of electrons. The existence condition for a solitary wave for a collisionless dusty plasma is re-examined. It is found that there is an upper limit of the possible Alfvenic Mach velocity, imposed by dust particles. The Mach number lies between l(z) and l(z)/root N(d), where l(z) is the directional cosine and N(d) is the dust particle charge density. In the collisional case, the same upper limit of the Mach velocity is found, and the solitary wave turns into an oscillating double layer. The damping scale and the size of the oscillation structure increase with increasing dust particle charge density. The damping scale and the size of the oscillation structure are estimated by using the virial theorem. (C) 2010 American Institute of Physics. [doi: 10.1063/1.3425867]-
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.titleObliquely propagating solitary kinetic Alfven wave in a collisional dusty plasma-
dc.typeArticle-
dc.contributor.college물리학과en_US
dc.identifier.doi10.1063/1.3425867-
dc.author.googleWoo, MHen_US
dc.author.googleRyu, CMen_US
dc.author.googleChoi, CRen_US
dc.relation.volume17en_US
dc.relation.issue5en_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.17, no.5-
dc.identifier.wosid000278182900070-
dc.date.tcdate2019-01-01-
dc.citation.number5-
dc.citation.titlePHYSICS OF PLASMAS-
dc.citation.volume17-
dc.contributor.affiliatedAuthorRyu, CM-
dc.identifier.scopusid2-s2.0-77952960400-
dc.description.journalClass1-
dc.description.journalClass1-
dc.description.wostc6-
dc.description.scptc7*
dc.date.scptcdate2018-10-274*
dc.type.docTypeArticle-
dc.subject.keywordAuthordusty plasmas-
dc.subject.keywordAuthorMach number-
dc.subject.keywordAuthorplasma Alfven waves-
dc.subject.keywordAuthorplasma collision processes-
dc.subject.keywordAuthorplasma sheaths-
dc.subject.keywordAuthorplasma solitons-
dc.subject.keywordAuthorplasma transport processes-
dc.relation.journalWebOfScienceCategoryPhysics, Fluids & Plasmas-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaPhysics-

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