Plasma Beta Stratification in the Solar Atmosphere: A Possible Explanation for the Penumbra Formation
Plasma Beta Stratification in the Solar Atmosphere: A Possible Explanation for the Penumbra Formation
复制标题
太阳大气中的等离子体贝塔层化：半影形成的可能解释
DOI：
10.3847/2041-8213/aa9988
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发表时间：
2017
期刊：
影响因子：
--
通讯作者：
P. Bourdin
中科院分区：
文献类型：
--
作者：
P. Bourdin
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Plasma beta is an important and fundamental physical quantity in order to understand plasma dynamics, particularly in the context of magnetically active stars, because it tells about the domination of magnetic versus thermodynamic processes on the plasma motion. We estimate the value ranges of plasma beta in different regions within the solar atmosphere and we describe a possible mechanism that helps forming a penumbra. For that we evaluate data from a 3D magnetohydrodynamic model of the solar corona above a magnetically active region. We compare our results with previously established data that is based on magnetic field extrapolations and that was matched for some observations. Our model data suggest that plasma beta in the photosphere should be considered to be larger than unity outside of sunspots. However, in the corona we also find that the beta value range reaches lower than previously thought, which coincides with a recent observation. We present an idea based on a gravity-driven process in a high-beta regime that might be responsible for the formation of the penumbra around sunspot umbra, where the vertical field strength reaches a given threshold. This process would also explain counter-Evershed flows. Regarding the thermal and magnetic pressure within the mixed-polarity solar atmosphere, including non-vertical magnetic field and quiet regions, plasma beta may reach unity at practically any height from the photosphere to the outer corona.
太阳黑子半影的形成 - 磁场特性
影响因子：
6.5
作者：
R. Rezaei;N. Bello Gonzalez;R. Schlichenmaier
通讯作者：
R. Schlichenmaier