Thermally damped waves in the solar corona

被引：0

作者：

Marcu, A. ^{[1
]}

Ballai, I. ^{[2
]}

机构：

[1] Univ Babes Bolyai, Dept Theoret & Computat Phys, M Kogalniceanu 1, R-3400 Cluj Napoca, Romania

[2] Univ Sheffield, Dept Math Appl, Solar Phys & Space Plasma Res Ctr, Sheffield, S Yorkshire, England

来源：

FLOWS, BOUNDARIES, INTERACTIONS | 2007年 / 934卷

关键词：

MHD; waves;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Waves observed by high resolution telescopes in the solar corona are subject to a rapid damping which could be due to non-ideal effects and/or transversal inhomogeneities. The attenuation of modes is currently used to determine, e.g. the value and structure of coronal magnetic field, a fundamental parameter which cannot be measured directly. Here we study the damping of linear MHD modes propagating in a stratified plasma in the presence of thermal conduction. For the chosen particular equilibrium we show the importance of the transversal motion in the process of wave damping.

引用

页码：64 / +

页数：2

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