Kelvin:Helmholtz Instability at the magnetopause: Solution for compressible plasmas
Kelvin:Helmholtz Instability at the magnetopause: Solution for compressible plasmas
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DOI:
10.1029/ja088ia02p00841
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发表时间:
1983-02
影响因子:
--
通讯作者:
Z. Pu;M. Kivelson
中科院分区:
文献类型:
--
作者:
Z. Pu;M. Kivelson
The Kelvin-Helmholtz (K-H) instability of a tangential discontinuity in a compressible plasma is reexamined in the linear magnetohydrodynamic (MHD) approximation. For fixed plasma conditions, two different kinds of surface waves (labeled F for fast and S for slow) may exist simultaneously with different tangential wave vectors k/sub t/. The surface waves can be excited only for a limited range of U, the relative flow speed of the plasmas on the two sides of the interface. Thus the instability requires U/sub c/m or approx. =U/sub i/, but the slow wave growth rate is small in comparison with both epsilon/sub F/ and epsilon/sub i/. Consequently, plasma compressibility is relatively ineffective in reducing the critical velocity for surface wave growth below that for an incompressible plasma.