首页> 外文会议>The 10th European Solar Physics Meeting Vol.2 Sep 9-14, 2002 Prague, Czech Republic >DAMPING OF CORONAL LOOP OSCILLATIONS BY RESONANT ABSORPTION OF QUASI-MODE KINK OSCILLATIONS
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DAMPING OF CORONAL LOOP OSCILLATIONS BY RESONANT ABSORPTION OF QUASI-MODE KINK OSCILLATIONS

机译:准模式扭结振荡的共振吸收对冠状环振荡的阻尼作用

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摘要

Damped quasi-mode kink oscillations in cylindrical flux tubes are capable of explaining the observed rapid damping of the coronal loop oscillations when the ratio of the inhomogeneity length scale to the radius of the loop is allowed to vary from loop to loop. They do not need to invoke anomalously low Reynolds numbers. The theoretical expressions for the decay time by Hollweg & Yang (1988) and Rud-erman & Roberts (2002) are used to estimate the ratio of the length scale of inhomogeneity compared to the loop radius for a collection of loop oscillations.
机译:圆柱状通量管中的阻尼准模式扭结振荡能够解释在不均匀长度标度与环路半径之比随环路变化时所观察到的冠状环路振荡的快速阻尼。他们不需要调用异常低的雷诺数。 Hollweg&Yang(1988)和Rud-erman&Roberts(2002)的衰减时间的理论表达式用于估计不均匀性的长度尺度与环路半径的比值,以收集环路振荡。

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