Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/36383
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dc.contributor.authorSingh, V-
dc.contributor.authorSingh, R N-
dc.date.accessioned2016-10-28T07:01:00Z-
dc.date.available2016-10-28T07:01:00Z-
dc.date.issued1989-04-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/36383-
dc.description37-43en_US
dc.description.abstractThe dispersion equation for whistler mode waves in the anisotropic plasma in the presence of parallel electrostatic field is derived. Using the realistic models of magnetospheric plasma and field parameters, the refractive index surfaces for whistler mode waves have been constructed. The presence of parallel electric field and anisotropy deform the refractive indeed surface and produce defocusing of whistler waves. The presence of parallel electric field induces an instability in the whistler mode waves which are found to depend on the magnitude and direction of the electrostatic field. It is concluded that the analysis of whistler wave records received on the ground is capable of accounting for the role of plasma anisotropy and the presence of parallel electric fields.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.18(2) [April 1989]en_US
dc.titlePropagation of whistler waves and their instability in the magenetosphereen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.18(2) [April 1989]

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