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dc.contributor.authorMeuris, Peter
dc.contributor.authorVerheest, F.
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2015-09-23T11:11:10Z
dc.date.accessioned2021-02-12T09:30:06Z
dc.date.available2015-09-23T11:11:10Z
dc.date.available2021-02-12T09:30:06Z
dc.date.issued1997
dc.identifier.citationPlanetary and Space Science, v.45/4, p.449-454, 1997, doi: 10.1016/S0032-0633(96)00155-9en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/486
dc.description.abstractThe linear dispersion law is given for a generalized Jeans-Buneman instability in the presence of a dust mass distribution. It is shown that this instability is easier to evoke when a reasonable power law mass distribution for the dust grains is assumed than for the mono-sized dust case. For Boltzmann distributed ions and electrons the dust-acoustic mode and the unstable Jeans mode are modified due to the self-gravitation and mass distribution. The frequency of the dust-acoustic mode is increased. For long wavelengths, a new stable mode occurs, due only to the dust mass distribution. The growth rate of the Jeans instability is increased, and the mode is extended beyond the usual wavelength domain. For high values of k a new instability arises, which is called the dust distribution instability.en_US
dc.language.isoenen_US
dc.subjectDusty plasmasen_US
dc.subjectJeans-Buneman instabilityen_US
dc.subjectDust mass distributionsen_US
dc.titleInfluence of dust mass distributions on generalized Jeans-Buneman instabilities in dusty plasmasen_US
dc.typeArticleen_US
dc.identifier.accession090995
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