Nonlinear Kink Oscillations of Coronal Magnetic Loops

被引:16
作者
Ruderman, M. S. [1 ,2 ]
Goossens, M. [3 ]
机构
[1] Univ Sheffield, SP2RC, Sheffield S3 7RH, S Yorkshire, England
[2] Russian Acad Sci, Space Res Inst IKI, Moscow, Russia
[3] Katholieke Univ Leuven, Dept Math, Ctr Math Plasma Astrophys, B-3001 Louvain, Belgium
关键词
Sun; Corona; Magnetic fields; Oscillations; ALFVEN WAVES; TRACE;
D O I
10.1007/s11207-013-0446-x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We studied nonlinear kink oscillations of a thin magnetic tube using the cold-plasma approximation. We assumed that the plasma density varies along the tube but does not vary in the radial direction. Using the regular perturbation method, we show that the nonlinearity does not affect the oscillation amplitude. We also calculated the nonlinear correction to the oscillation frequency, which is proportional to the oscillation amplitude squared. As an example, we considered nonlinear oscillations of a coronal magnetic loop of half-circle shape in an isothermal atmosphere with equal plasma temperatures inside and outside the loop.
引用
收藏
页码:1999 / 2020
页数:22
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