Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/35889
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dc.contributor.authorSingh, D P-
dc.contributor.authorPrakash, Ram-
dc.date.accessioned2016-10-20T08:48:28Z-
dc.date.available2016-10-20T08:48:28Z-
dc.date.issued1994-08-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/35889-
dc.description288-292en_US
dc.description.abstractThe impact of solar wind distorted dipolar field on magnetospheric parameters and quiet time parallel whistler mode propagation has been studied. It is shown that in the compressed dipolar field the resonant velocity of energetic electrons as well as their integral flux, increase above their values in a dipole field. Because of this, the temporal wave growth and power gain of whistler mode waves are increased significantly. The increments in temporal wave growth and power gain are directly proportional to the solar wind intensity, and the effects are more pronounced at higher L shells than at lower L shells.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.23(4) [August 1994]en_US
dc.titleWhistler wave amplification by compressed dipolar fielden_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.23(4) [August 1994]

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