期刊
SPACE SCIENCE REVIEWS
卷 149, 期 1-4, 页码 255-282出版社
SPRINGER
DOI: 10.1007/s11214-009-9560-3
关键词
Sun; Solar corona; MHD waves
资金
- [GOA/2009-009]
In this work we review the efforts that have been done to study the excitation of the standing fast kink body mode in coronal loops. We mainly focus on the time-dependent problem, which is appropriate to describe flare or CME induced kink oscillations. The analytical and numerical studies in slab and cylindrical loop geometries are reviewed. We discuss the results from very simple one-dimensional models to more realistic (but still simple) loop configurations. We emphasise how the results of the initial value problem complement the eigenmode calculations. The possible damping mechanisms of the kink oscillations are also discussed.
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