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arXiv · 1706.08878

The causes of quasi-homologous CMEs

Lijuan Liu·Yuming Wang·Rui Liu·Zhenjun Zhou·M. Temmer·J. K. Thalmann·Jiajia Liu·Kai Liu·Chenglong Shen·Quanhao Zhang·A. M. Veronig
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Abstract

In this paper, we identified the magnetic source locations of 142 quasi- homologous (QH) coronal mass ejections (CMEs), of which 121 are from solar cycle (SC) 23 and 21 from SC 24. Among those CMEs, 63% originated from the same source location as their predecessor (defined as S-type), while 37% origi- nated from a different location within the same active region as their predecessor (defined as D-type). Their distinctly different waiting time distribution, peaking around 7.5 and 1.5 hours for S- and D-type CMEs, suggests that they might involve different physical mechanisms with different characteristic time scales. Through detailed analysis based on non-linear force free (NLFF) coronal mag- netic field modeling of two exemplary cases, we propose that the S-type QH CMES might involve a recurring energy release process from the same source location (by magnetic free energy replenishment), whereas the D-type QH CMEs can happen when a flux tube system disturbed by a nearby CME.

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Lijuan Liu, Yuming Wang, Rui Liu, Zhenjun Zhou, M. Temmer, J. K. Thalmann, Jiajia Liu, Kai Liu, Chenglong Shen, Quanhao Zhang, A. M. Veronig. 2017-06-27. The causes of quasi-homologous CMEs. https://doi.org/10.3847/1538-4357%2Faa7d56

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