Please use this identifier to cite or link to this item:
|Title:||Whistler wave amplification by compressed dipolar field|
|Authors:||Singh, D P|
|Abstract:||The 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.|
|ISSN:||0975-105X (Online); 0367-8393 (Print)|
|Appears in Collections:||IJRSP Vol.23(4) [August 1994]|
Items in NOPR are protected by copyright, with all rights reserved, unless otherwise indicated.