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dc.contributor.authorVerheest, F.
dc.contributor.authorHellberg, M.A.
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2015-09-11T11:16:16Z
dc.date.accessioned2021-02-12T09:28:12Z
dc.date.available2015-09-11T11:16:16Z
dc.date.available2021-02-12T09:28:12Z
dc.date.copyrightCC BY 4.0
dc.date.issued2007
dc.identifier.citationAstrophysics and Space Science Transactions, v.3, p.15-20, 2007, doi: 10.5194/astra-3-15-2007en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/390
dc.description.abstractNecessary conditions are discussed for the possible generation of large solitary acoustic modes in plasmas with one or more ion species which are hotter than some or all of the electron species. The analysis is based on a fluid dynamic approach. It is found that in most of these configurations the existence ranges for the solitary wave velocities are very narrow and close to one of the thermal velocities. In the latter situation, linear Landau damping may prevent the generation of nonlinear structures. The analysis indicates that both inertial and thermal effects for the ions need to be kept in the description, thus rendering an analytical investigation much more intricate.en_US
dc.language.isoenen_US
dc.subjectAcoustic solitonsen_US
dc.subjectMagnetosphericen_US
dc.subjectSpace plasmaen_US
dc.subjectSolitary wavesen_US
dc.subjectPlasmaen_US
dc.subjectHot ionsen_US
dc.titleNecessary conditions for the generation of acoustic solitons in magnetospheric and space plasmas with hot ionsen_US
dc.typeArticleen_US
dc.identifier.accession090885
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