Detection of waves in the solar corona: Kink or Alfven?

被引：223
|
作者：
Van Doorsselaere, T. [1 ]
Nakariakov, V. M. [1 ]
Verwichte, E. [1 ]
机构：
[1] Univ Warwick, Ctr Fus Space & Astrophys, Dept Phys, Coventry CV4 7AL, W Midlands, England
来源：
ASTROPHYSICAL JOURNAL LETTERS | 2008年 / 676卷 / 01期
基金：
英国科学技术设施理事会; 英国工程与自然科学研究理事会;
关键词：
MHD; sun : corona; sun : oscillations;
D O I：
10.1086/587029
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Recently, the omnipresence of waves has been discovered in the corona using the CoMP instrument. We demonstrate that the observational findings can be explained in terms of guided kink magnetoacoustic modes. The interpretation of the observations in terms of Alfven waves is shown to be inconsistent with MHD wave theory. The implications of the interpretation in terms of kink waves are discussed.
引用
收藏
页码：L73 / L75
页数：3
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