Whistler precursor and intrinsic variability of quasi-perpendicular shocks

被引:2
|
作者
Granit, Gilad [1 ]
Gedalin, Michael [1 ]
机构
[1] Ben Gurion Univ Negev, Dept Phys, Beer Sheva, Israel
基金
以色列科学基金会;
关键词
astrophysical plasmas; plasma nonlinear phenomena; space plasma physics; NONLINEAR-WAVES; NONSTATIONARITY;
D O I
10.1017/S0022377818000107
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 structure of a whistler precursor in a quasi-perpendicular shock is studied within two-fluid approach in one-dimensional case. The complete set of equations is reduced to the KdV equation, if no dissipation is included. With a phenomenological resistive dissipation the structure is described with the KdV-Burgers equation. The shock profile is intrinsically time dependent. For sufficiently strong dissipation, temporal evolution of a steepening profile results in generation of a stationary decaying whistler ahead of the shock front. With the decrease of the dissipation parameter, whistler wave trains begin to detach and propagate toward the upstream and the ramp is weakly time dependent. In the weakly dissipative regime the shock front experiences reformation.
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页数:14
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