A Triggering of Solar Flare by Magnetosonic Waves in a Neutral Sheet Plasma

J. Sakai, H. Washimi
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引用次数: 30

Abstract

A theoroetical model of the triggering of a solar flare by magnetosonic waves in a neutral sheet plasma is discussed. It is shown that the ponderomotive force due to the magnetosonic waves strongly excites the plamsa convection flow in the magnetic neutral sheet which in turn enhances the tearing instability. The system of basic equations for the tearing mode, including the time-averaged nonlinear effects due to the growth time of the instability is shortened to about 100 s for reasonable magnetosonic wave intensity.
中性片状等离子体中磁声波对太阳耀斑的触发
讨论了中性片状等离子体中磁声波触发太阳耀斑的理论模型。结果表明,磁声波引起的磁动势强烈地激发了磁中性片内的等离子体对流流动,从而增强了磁中性片的撕裂不稳定性。在合理的磁声波强度下,将撕裂模式的基本方程系统(包括不稳定性增长时间平均非线性效应)缩短到100 s左右。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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