Excitation of Kelvin Helmholtz instability by an ion beam in a plasma with negatively charged dust grains

被引:2
|
作者
Rani, Kavita [1 ]
Sharma, Suresh C. [2 ]
机构
[1] Bhagwan Parshuram Inst Technol, Dept Appl Phys, Sect 17, New Delhi 110089, India
[2] DTU, Dept Appl Phys, New Delhi 110042, India
关键词
SOLAR-WIND; TRANSPORT; WAVES; MODES;
D O I
10.1063/1.4913230
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
An ion beam propagating through a magnetized dusty plasma drives Kelvin Helmholtz Instability (KHI) via Cerenkov interaction. The frequency of the unstable wave increases with the relative density of negatively charged dust grains. It is observed that the beam has stabilizing effect on the growth rate of KHI for low shear parameter, but for high shear parameter, the instability is destabilized with relative density of negatively charged dust grains. (C) 2015 AIP Publishing LLC.
引用
收藏
页数:5
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