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An approximate solution of the parallel whistler-mode dispersion equation in a weakly relativistic plasma

S S Sazhin, A E Sumner, N M Temme, F Gugic1993年Plasma Physics and Controlled FusionIF 2.2出版社

A new approximate solution of the parallel whistler-mode dispersion equation in a weakly relativistic plasma is obtained under the assumption that the real part of the wave refractive index, N, predicted by this solution is close to the value of N predicted by the solution of the corresponding non-relativistic dispersion equation. Both the values of N and the values of the increment of wave growth or damping are closer to those obtained by numerical solution of the weakly relativistic dispersion equations than previously suggested approximations. The accuracy of the obtained solution increases with decreasing electron density, and/or anisotropy of the electron distribution function, and/or electron energy.

日本語訳

弱相対論的プラズマにおける平行伝播ホイスラー・モード分散方程式の新しい近似解が、この解によって予測される波動屈折率Nの実部が、対応する非相対論的分散方程式の解によって予測されるNの値に近いという仮定の下で得られた。Nの値および波動の成長または減衰の増分の値は、いずれも、従来提案された近似解によるものよりも、弱相対論的分散方程式の数値解によって得られる値に近い。得られた解の精度は、電子密度、および/または電子分布関数の異方性、および/または電子エネルギーの減少とともに向上する。

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