Linear and nonlinear dynamics of current-driven waves in dusty plasmas

被引:1
作者
Ahmad, Ali [1 ,2 ,3 ]
Shan, S. Ali [1 ,3 ]
Haque, Q. [1 ,3 ]
Saleem, H. [1 ,2 ]
机构
[1] NCP, Islamabad 44000, Pakistan
[2] CIIT Ctr Hlth Res, Dept Phys, Islamabad, Pakistan
[3] PINSTECH, Theoret Plasma Phys Div, Islamabad, Pakistan
关键词
DRIFT WAVES; SOLAR-WIND; ELECTRONS; DISTRIBUTIONS; INSTABILITY; MODES; ION;
D O I
10.1063/1.4754282
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
The linear and nonlinear dynamics of a recently proposed plasma mode of dusty plasma is studied using kappa distribution for electrons. This electrostatic wave can propagate in the plasma due to the sheared flow of electrons and ions parallel to the external magnetic field in the presence of stationary dust. The coupling of this wave with the usual drift wave and ion acoustic wave is investigated. D'Angelo's mode is also modified in the presence of superthermal electrons. In the nonlinear regime, the wave can give rise to dipolar vortex structures if the shear in flow is weaker and tripolar vortices if the flow has steeper gradient. The results have been applied to Saturn's magnetosphere corresponding to negatively charged dust grains. But the theoretical model is applicable for positively charged dust as well. This work will be useful for future observations and studies of dusty environments of planets and comets. (C) 2012 American Institute of Physics. [http://dx.doi.org/10.1063/1.4754282]
引用
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页数:7
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