Kink mode m=1 in magnetic tube with discontinuous magnetic field

被引:4
作者
Cheremnykh, O. K. [1 ]
Kryshtal, A. N.
Tkachenko, A. A.
机构
[1] Space Res Inst NSAU, 40-1 Acad Glushkov Ave,MSP 03680, UA-187 Kiev, Ukraine
关键词
MHD approach; Magnetic flux tubes; Kink mode; Plasma stability; Condition of propagation of plasma waves; FLUX TUBES; WAVES; PLASMA;
D O I
10.1016/j.asr.2017.05.026
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
In this paper, we study conditions of realization and stability of kink modes with azimuthal wave numbers m = +/- 1 in cylindrical plasma flex with twisted magnetic field and homogeneous current along its axis. We assume permanent axial magnetic field both inside and outside the flex, surrounded by currentless plasma. Azimuthal magnetic field decreases inversely proportional to the distance from the boundary beyond the flex. We derived dispersion equations for stable and unstable modes in approximation of "thin" plasma flex. The analysis of equations has been provided for the case of discontinuous axial magnetic field on flex's boundary. Conditions of propagation of wave modes have been defined. It was shown, that unstable modes can be implemented in certain interval of longitudinal wavenumbers. Results can be applied for the interpretation of solar magnetic tubes behavior, using measurements, provided by spacecrafts. (C) 2017 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:603 / 610
页数:8
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