Kink mode m = 1 in a thin plasma filament with discontinuous vertical magnetic field
- 作者: Cheremnykh O.K.1, Kryshtal A.N.1, Tkachenko A.A.1
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隶属关系:
- Institute for Cosmic Research
- 期: 卷 33, 编号 3 (2017)
- 页面: 95-110
- 栏目: Solar Physics
- URL: https://ogarev-online.ru/0884-5913/article/view/177958
- DOI: https://doi.org/10.3103/S0884591317030023
- ID: 177958
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详细
In this paper, we study the conditions of realization and stability of kink modes with azimuthal wave numbers m = ±1 in a cylindrical plasma filament with a twisted magnetic field and a homogeneous current along its axis. We assume that there are vertical constant magnetic fields inside and outside of the filament; the filament is surrounded by current-free plasma; and outside of its boundary, the azimuthal magnetic field decreases inversely in proportion to the distance from the filament’s border. The dispersion equations for stable and unstable modes are obtained in the approximation of “thin” plasma filament. The analysis of the equations for the case of discontinuous vertical magnetic field at the filament’s boundary is provided. The conditions of propagation of the wave modes have been defined. We have obtained that the unstable modes with m = ±1 cannot be realized. The results of this work can be applied to the interpretation of the solar magnetic flux tubes’ behavior using measurements provided by the spacecrafts.
作者简介
O. Cheremnykh
Institute for Cosmic Research
编辑信件的主要联系方式.
Email: oleg.cheremnykh@gmail.com
乌克兰, Kyiv, 03143
A. Kryshtal
Institute for Cosmic Research
Email: oleg.cheremnykh@gmail.com
乌克兰, Kyiv, 03143
A. Tkachenko
Institute for Cosmic Research
Email: oleg.cheremnykh@gmail.com
乌克兰, Kyiv, 03143
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