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On Making Magnetic-flux-rope Ω Loops for Solar Bipolar Magnetic Regions of All Sizes by Convection Cells
The Astrophysical Journal Letters ( IF 7.9 ) Pub Date : 2020-10-18 , DOI: 10.3847/2041-8213/abbade
Ronald L. Moore 1, 2 , Sanjiv K. Tiwari 3, 4 , Navdeep K. Panesar 3, 4 , Alphonse C. Sterling 2
Affiliation  

We propose that the flux-rope Ω loop that emerges to become any bipolar magnetic region (BMR) is made by a convection cell of the Ω-loop’s size from initially horizontal magnetic field ingested through the cell’s bottom. This idea is based on (1) observed characteristics of BMRs of all spans (∼1000 to ∼200,000 km), (2) a well-known simulation of the production of a BMR by a supergranule-sized convection cell from horizontal field placed at cell bottom, and (3) a well-known convection-zone simulation. From the observations and simulations, we (1) infer that the strength of the field ingested by the biggest convection cells (giant cells) to make the biggest BMR Ω loops is ∼10 3 G, (2) plausibly explain why the span and flux of the biggest observed BMRs are ∼200,000 km and ∼10 22 Mx, (3) suggest how giant cells might also make “failed-BMR” Ω loops that populate the upper convection zone with horizontal field, from which smaller convection cells make BMR Ω loops ...

中文翻译:

对流电池制作各种尺寸太阳双极磁场区域的磁通量Ω环的研究

我们提出,通向具有任何Ω环大小的对流单元的磁通量Ω环路是由通过该单元底部吸收的初始水平磁场构成的,该对流单元的尺寸为Ω环。这个想法是基于(1)观察到的所有跨度(〜1000至〜200,000 km)的BMR的特征,(2)一个超模拟的对流单元通过放置在水平方向上的水平场产生BMR的众所周知的模拟。单元底部,以及(3)众所周知的对流区模拟。从观察和模拟中,我们(1)推断出最大对流单元(巨型细胞)摄取的形成最大BMRΩ环的电场强度约为10 3 G,(2)合理地解释了为何跨度和通量观测到的最大BMR约为200,000 km和10 22 Mx,
更新日期:2020-10-19
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