PROPAGATION OF DISTURBANCES IN SOLAR CHROMOSPHERE-CORONA
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摘要: 为了模拟太阳色球层、过渡层和日冕中扰动的传播特征,本文在一自洽的非等温、非均匀等离子体初态下,应用二维时变可压缩磁流体动力学模拟,数值研究了过渡层附近局地加热引起的扰动传播过程.结果表明,扰动分别以局地快磁流波速度向四周传播,数值模拟结果与局地快磁流波推算结果符合得很好,其特征可以解释SOHO/EIT观测到的波动事件.Abstract: In order to simulate the propagation characteristics of disturbances in solar chromosphere, transition layer and corona, we discuss numerically the propagation process of a disturbance produced by local heating in vicinity of transition layer, by adopting a 2-dimensional MHD simulation under a self-consistent non-isothermal, non-uniform initial state. The results indicate that the disturbance propagates to ambient plasma with a speed of local fast MHD wave. We find the numerical results can fit in with that computed via local fast MHD wave, its characteristics can explain wave events observed by SOHO/EIT.
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Key words:
- Corona /
- Chromosphere /
- MHD wave
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