Oblique whistler waves generated in cold plasma by relativistic electron beams

被引：13
|
作者：
Ciurea-Borcia, R [1 ]
Matthieussent, G
Le Bel, E
Simonet, F
Solomon, J
机构：
[1] Alexandru Ioan Cuza Univ, Fac Phys, Iasi 6600, Romania
[2] Univ Paris 11, Phys Gaz & Plasmas Lab, CNRS, UMR 8578, F-91405 Orsay, France
[3] CEA, DIF, F-91680 Bruyeres Le Chatel, France
[4] Univ Paris 11, CNRS, Inst Astrophys Spatiale, F-91405 Orsay, France
来源：
PHYSICS OF PLASMAS | 2000年 / 7卷 / 01期
关键词：
D O I：
10.1063/1.873804
中图分类号：
O35 [流体力学]; O53 [等离子体物理学];
学科分类号：
070204 ; 080103 ; 080704 ;
摘要：
Parallel and oblique propagation of whistler waves generated by relativistic electron beams are examined. From the general dispersion equation one derives the analytical formula for the linear growth rate in the relativistic case. The growth rate is computed for realistic plasma parameters, using two distinct distribution functions for the hot electron population. The results of the present paper can explain phenomena occurring in space plasmas where relativistic electrons are present. (C) 2000 American Institute of Physics. [S1070-664X(00)00701-1].
引用
收藏
页码：359 / 370
页数：12
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