Nonlinear resonant absorption of fast magnetoacoustic waves due to coupling into slow continue in the solar atmosphere

被引:10
作者
Erdélyi, R
Ballai, I
Goossens, M
机构
[1] Univ Sheffield, Dept Appl Math, Space & Atmosphere Res Ctr, Sheffield S3 7RH, S Yorkshire, England
[2] Katholieke Univ Leuven, Ctr Plasma Astrophys, B-3001 Heverlee, Belgium
关键词
magnetohydrodynamics (MHD); Sun : oscillations; Sun : atmosphere;
D O I
10.1051/0004-6361:20010105
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Nonlinear resonant absorption of fast magnetoacoustic (FMA) waves in inhomogeneous weakly dissipative, isotropic and anisotropic plasmas in static and steady equilibria is studied. Both isotropic and anisotropic plasmas are considered and for the background equilibrium state 1D planar static and steady models are used. The equilibrium configuration consists of three layers, where an inhomogeneous: magnetised plasma slab is surrounded by two homogeneous magnetised semi-infinite plasma regions. The propagating FMA waves are partly absorbed due to coupling to local nonlinear slow magnetohydrodynamic (MHD) waves in the inhomogeneous layer, and are partly reflected. The coefficient of wave energy resonant absorption is derived using two simplifying assumptions (i) weak nonlinearity and (ii) the thickness: of the inhomogeneous layer is small compared to the wavelength of the waves, i.e. the so-called long-wavelength approximation is used.
引用
收藏
页码:662 / 675
页数:14
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