Generation of whistler mode in a relativistic plasma

被引：0
|
作者：
N. K. Deka
B. J. Saikia
K. S. Goswami
机构：
[1] Cotton College,Department of Physics
[2] Centre of Plasma Physics,undefined
来源：
Pramana | 2008年 / 70卷
关键词：
Energy up-conversion process; weak turbulence theory; 52.35.-g; 52.35.Ra; 52.35.Nx;
D O I：
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学科分类号：
摘要：
This paper contains the plasma maser interaction between high frequency nonresonant whistler R-mode and low frequency resonant ion acoustic mode in a relativistic plasma. It shows that the whistler R-mode grows through the plasma maser interaction between the relativistic electrons and the ion acoustic fluctuation.
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