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Current-less solar wind driven dust acoustic instability in cometary plasma

dc.contributor.authorVranjes, J.
dc.date2011
dc.date.accessioned2016-03-29T12:43:54Z
dc.date.available2016-03-29T12:43:54Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3149
dc.descriptionA quantitative analysis is presented of the dust acoustic wave instability driven by the solar and stellar winds. This is a current-less kinetic instability which develops in permeating plasmas, i.e., when one quasi-neutral electron-ion wind plasma in its propagation penetrates through another quasi-neutral plasma which contains dust, electrons, and ions.
dc.languageeng
dc.titleCurrent-less solar wind driven dust acoustic instability in cometary plasma
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeDust acoustic instability
dc.subject.freeDust acoustic waves
dc.subject.freeElectron ions
dc.subject.freeKinetic instability
dc.subject.freeQuasi-neutral plasma
dc.subject.freeStellar wind
dc.subject.freeAcoustics
dc.subject.freeDust
dc.subject.freePlasma stability
dc.subject.freePlasmas
dc.subject.freeSolar wind
dc.subject.freePlasma diagnostics
dc.source.titlePhysics of Plasmas
dc.source.volume18
dc.source.issue8
dc.source.page84501
Orfeo.peerreviewedYes
dc.identifier.doi10.1063/1.3619819
dc.identifier.scopus2-s2.0-80052406046


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