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Cited 6 time in webofscience Cited 6 time in scopus
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dc.contributor.authorAnurai Panwar-
dc.contributor.authorRizvi, H-
dc.contributor.authorRyu, CM-
dc.date.accessioned2015-06-25T03:22:31Z-
dc.date.available2015-06-25T03:22:31Z-
dc.date.created2014-03-03-
dc.date.issued2013-05-
dc.identifier.issn1070-664X-
dc.identifier.other2015-OAK-0000029019en_US
dc.identifier.urihttps://oasis.postech.ac.kr/handle/2014.oak/12622-
dc.description.abstractLarge amplitude inertial compressional Alfvenic shock and solitary waves in magnetohydrodynamic plasmas are investigated. Dispersive effect caused by non-ideal electron inertia currents perpendicular to the ambient magnetic field can balance the nonlinear steepening of waves leading to the formation of a soliton. A Sagdeev-potential formalism is employed to derive an energy-balance like equation. The range of allowed values of the soliton speed, M (Mach number), plasma beta (ratio of the plasma thermal pressure to the pressure in the confining magnetic field), and electron inertia, wherein solitary waves may exist, are determined. Depth of the potential increases with increasing the Mach number and plasma beta, however decreases with the increasing electron inertia. The height of soliton increases with increasing in Mach number and decreases with plasma beta. And with increasing electron inertial length, the width of soliton increases. The electron-ion collisional dissipation results a dissipative inertial compressional Alfven wave, which can produce a shock like structure and can efficiently accelerate ions to the order of the local Alfven velocity. The shock height increases with the increasing collision frequency, but shock height decreases with increasing plasma beta. (C) 2013 AIP Publishing LLC.-
dc.description.statementofresponsibilityopenen_US
dc.languageEnglish-
dc.publisherAIP Publishing-
dc.relation.isPartOfPHYSICS OF PLASMAS-
dc.rightsBY_NC_NDen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/2.0/kren_US
dc.titleLarge amplitude inertial compressional Alfvenic shock and solitary waves, and acceleration of ions in magnetohydrodynamic plasmas-
dc.typeArticle-
dc.contributor.college물리학과en_US
dc.identifier.doi10.1063/1.4803064-
dc.author.googlePanwar, Aen_US
dc.author.googleRizvi, Hen_US
dc.author.googleRyu, CMen_US
dc.relation.volume20en_US
dc.relation.issue5en_US
dc.relation.startpage52103en_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.20, no.5, pp.52103-
dc.identifier.wosid000320000000003-
dc.date.tcdate2019-01-01-
dc.citation.number5-
dc.citation.startPage52103-
dc.citation.titlePHYSICS OF PLASMAS-
dc.citation.volume20-
dc.contributor.affiliatedAuthorRyu, CM-
dc.identifier.scopusid2-s2.0-84878938141-
dc.description.journalClass1-
dc.description.journalClass1-
dc.description.wostc4-
dc.description.scptc4*
dc.date.scptcdate2018-10-274*
dc.type.docTypeArticle-
dc.subject.keywordPlusELECTRON INERTIA-
dc.subject.keywordPlusCOLLISIONAL MAGNETOPLASMA-
dc.subject.keywordPlusRECONNECTION-
dc.relation.journalWebOfScienceCategoryPhysics, Fluids & Plasmas-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaPhysics-

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