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arXiv · 1712.07833

A Quantity Characterising Variation of Observed Magnetic Twist of Solar Active Regions

Yu Gao
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Abstract

An alternative parameter $R_{J_z}$ is introduced as the ratio of one of two kinds of opposite-sign current to the total current and investigate the relationship between the quantity and the hemispheric sign rule of helicity (HSR) that is established by a series of previous statistical studies. The classification of current in each hemisphere is according to the following rule: If the product of the current and the corresponding longitudinal field component contributes a consistent sign with reference to the HSR, it is called "HSR-compliant" current, or else it is called "HSR-noncompliant" current. Firstly, the consistence between the butterfly diagram of the $R_{J_z}$ and the current helicity was obtained in a statistical study. Active regions with $R_{J_z}$ smaller than 0.5 tend to obey the HSR whereas those with $R_{J_z}$ greater than 0.5 tend to disobey the HSR. The "HSR-compliant" current systems have 60\% probability of realization compared to 40\% of "HSR-noncompliant" current systems. Overall, the HSR is violated for active regions in which the "HSR-noncompliant" current is greater than the "HSR-compliant" current. Secondly, the $R_{J_z}$ parameter was subsequently used to study the evolution of current systems in the case analyses of flare-productive active regions NOAA AR 11158 and 11283. It is found that there were "$R_{J_z}$-quasi-stationary" phase that is relatively flare quiescent and "$R_{J_z}$-dynamic" phase that is covered by the occurrence of large flares.

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Yu Gao. 2017-12-21. A Quantity Characterising Variation of Observed Magnetic Twist of Solar Active Regions. https://arxiv.org/abs/1712.07833

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