Nonlinear damping of fast waves and plasma heating in the solar corona

被引：0
|
作者：
Voitenko, Y
Goossens, M
机构：
[1] Katholieke Univ Leuven, Ctr Plasma Astrophys, B-3001 Heverlee, Belgium
[2] Main Astron Observ, UA-03680 Kiev 127, Ukraine
来源：
RECENT INSIGHTS INTO THE PHYSICS OF THE SUN AND HELIOSPHERE: HIGHLIGHTS FROM SOHO AND OTHER SPACE MISSIONS | 2001年 / 203期
关键词：
D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A nonlinear mechanism for the damping of fast magnetoacoustic wave in the solar corona is studied. It is shown that the nonlinear coupling of finite-amplitude fast waves to small-scale Alfven waves can be much faster than damping mechanisms involving classic transport coefficients.
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收藏
页码：517 / 519
页数：3
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