Resonant Absorption of Magnetohydrodynamic Body Modes under Photospheric Conditions

D. J. Yu
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Abstract

Observations reveal that surface and body modes exist in solar pores under photospheric conditions. While the effects of resonant absorption on photospheric surface modes are well established, its effect on body modes is not known yet. In this paper, we investigate resonant absorption for the body modes under photospheric conditions. We numerically solve the dispersion relation induced by thin boundary approximation and obtain the wave dispersion curves and damping rates of three arbitrarily chosen body modes for sausage and kink waves, respectively. The results show that resonant absorption for the body modes is weaker than for the slow surface modes in both cusp and Alfvén continua. The damping behavior of body modes is similar to slow surface modes while the higher body mode has stronger resonant absorption.
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光层条件下磁流体动力体模的共振吸收
观测结果表明,在光层条件下,太阳孔隙中存在面模和体模。共振吸收对光层表面模式的影响已经得到证实,但对体模式的影响尚不清楚。本文研究了光层条件下体模的共振吸收。我们对薄边界近似引起的频散关系进行了数值求解,并分别得到了任意选取的三种体模的香肠波和扭结波的波频散曲线和阻尼率。结果表明,在尖顶波和阿尔弗文连续波中,体模的共振吸收都弱于慢面模。体模的阻尼行为与慢速表面模相似,而较高的体模具有更强的共振吸收。
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