Coronal dynamics and heating theories

被引：0
|
作者：
Gudiksen, Boris V. [1 ]
机构：
[1] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway
来源：
ADVANCES IN SPACE RESEARCH | 2009年 / 43卷 / 01期
关键词：
Magnetohydrodynamics and plasmas; Solar corona; AB-INITIO APPROACH; LOOPS; SUN; ULTRAVIOLET; REGIONS; MODELS; WAVES; TRACE;
D O I：
10.1016/j.asr.2008.05.012
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
A large number of coronal heating theories have been proposed and most of them can be labeled as AC or DC heating theories. Here a short description of these two main theories is given, and the results of a DC heating model simulation is explained in more detail. As a result of that model, arguments are given for putting emphasis on launching a very fast spectrograph, ideally a imaging spectrograph as soon as possible. (C) 2008 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码：108 / 112
页数：5
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