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dc.contributor.authorTagare, S.G.
dc.contributor.authorSingh, S.V.
dc.contributor.authorReddy, R.V.
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2015-08-25T11:13:51Z
dc.date.accessioned2021-02-12T09:27:42Z-
dc.date.available2015-08-25T11:13:51Z
dc.date.available2021-02-12T09:27:42Z-
dc.date.issued2004
dc.identifier.citationNonlinear Processes in Geophysics, v.11, p.215-218, 2004.en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/286-
dc.description.abstractSmall amplitude electron - acoustic solitons are studied in a magnetized plasma consisting of two types of electrons, namely cold electron beam and background plasma electrons and two temperature ion plasma. The analysis predicts rarefactive solitons. The model may provide a possible explanation for the perpendicular polarization of the low-frequency component of the broadband electrostatic noise observed in the Earth's magnetotail.en_US
dc.language.isoenen_US
dc.subjectSmall amplitude electronen_US
dc.subjectEarth's magnetotailen_US
dc.subjectElectrostatic noiseen_US
dc.subjectElectron acoustic solitonsen_US
dc.titleElectron acoustic solitons in the Earth's magnetotailen_US
dc.typeArticleen_US
dc.identifier.accession090775
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