Stability of the kinetic Alfven wave in a current-less plasma

被引:1
|
作者
Sreekala, G. [1 ]
Sebastian, Sijo [1 ]
Michael, Manesh [1 ]
Abraham, Noble P. [1 ]
Renuka, G. [2 ]
Venugopal, Chandu [1 ]
机构
[1] Mahatma Gandhi Univ, Sch Pure & Appl Phys, Kottayam 686560, Kerala, India
[2] Kerala State Council Sci Technol & Environm, Thiruvananthapuram 695004, Kerala, India
关键词
Kinetic Alfven wave; Two potential theory; Stability; Multi-ion plasma; AURORAL ELECTRON ACCELERATION; COMET GIACOBINI-ZINNER; ELECTROMAGNETIC-WAVES; INSTABILITY DRIVEN; SOLAR-WIND; IONS; EXCITATION; TURBULENCE;
D O I
10.1016/j.asr.2015.03.016
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The two potential theory of Hasegawa has been used to derive the dispersion relation for the kinetic Alfven wave (KAW) in a plasma composed of hydrogen, oxygen and electrons. All three components have been modeled by ring distributions (obtained by subtracting two Maxwellian distributions with different temperatures) with the hydrogen and electrons drifting, respectively, with velocities V-dH and V-de. For the most general case, the dispersion relation is a polynomial equation of order five; it reduces to a relation which supports only one mode when V-dH = 0. For typical parameters at comet Halley, we find that both V-dH and V-de can drive the wave unstable; the KAW is thus driven unstable in a current-less plasma. Such an instability was found for the ion acoustic wave by Vranjes et al. (2009). (C) 2015 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:2519 / 2525
页数:7
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