Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456789/1038
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dc.contributor.authorKakad, Amar
dc.contributor.authorKakad, Bharati
dc.contributor.authorAnekallu, Chandrasekhar
dc.contributor.authorLakhina, G.S.
dc.contributor.authorYoshiharu, Omura
dc.contributor.authorFazakerley, Andrew
dc.date.accessioned2017-11-03T10:15:37Z
dc.date.accessioned2021-02-12T10:02:20Z-
dc.date.available2017-11-03T10:15:37Z
dc.date.available2021-02-12T10:02:20Z-
dc.date.issued2016
dc.identifier.citationJGR, 121, doi:10.1002/2016JA022365en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/1038-
dc.description.abstractWe modeled Cluster spacecraft observations of slow electrostatic solitary waves (SESWs) in the Earth’s northern plasma sheet boundary layer (PSBL) region on the basis of nonlinear fluid theory and fluid simulation. Various plasma parameters observed by the Cluster satellite at the time of the SESWs were examined to investigate the generation process of the SESWs. The nonlinear fluid model shows the coexistence of slow and fast ion acoustic waves and the presence of electron acoustic waves in the PSBL region. The fluid simulations, performed to examine the evolution of these waves in the PSBL region, showed the presence of an extra mode along with the waves supported by the nonlinear fluid theory. This extra mode is identified as the Buneman mode, which is generated by relative drifts of ions and electrons. A detailed investigation of the characteristics of the SESWs reveals that the SESWs are slow ion acoustic solitary waves.en_US
dc.language.isoenen_US
dc.subjectSlow electrostatic solitary wavesen_US
dc.subjectPlasma sheeten_US
dc.subjectIon acoustic solitary wavesen_US
dc.subjectSolitary wavesen_US
dc.subjectBoundary layeren_US
dc.titleSlow electrostatic solitary waves in Earth’s plasma sheet boundary layeren_US
dc.typeArticleen_US
dc.identifier.accession091580
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