Current-driven Alfv,n waves in dusty magnetospheric plasmas

被引:1
作者
Shan, S. Ali [1 ,2 ,3 ]
Haque, Q. [1 ,2 ,3 ]
Saleem, H. [1 ,3 ]
机构
[1] NCP, Islamabad 44000, Pakistan
[2] PINSTECH, Theoret Plasma Phys Div, Islamabad, Pakistan
[3] PIEAS, Islamabad, Pakistan
关键词
Current-driven instability; Sheared flow instability; SOLAR-WIND; ION WAVES; INSTABILITY; TURBULENCE; MODES;
D O I
10.1007/s10509-013-1658-0
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It is shown that the sheared flow of electrons and ions in the presence of heavy stationary dust gives rise to unstable Alfv,n waves. The coupling of newly studied low frequency electrostatic current-driven mode with the electromagnetic Alfv,n and drift waves is investigated. The instability conditions and the growth rates of both inertial and kinetic Alfv,n waves are estimated. The theoretical model is applied to the night side boundary regions of Jupiter's magnetosphere which contain positive dust. The growth rates increase with increase in sheared flow speed. In the nonlinear regime, both inertial and kinetic Alfv,n waves form dipolar vortices whose speed and amplitude depend upon the magnitude of the zero-order current.
引用
收藏
页码:285 / 291
页数:7
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