The initiation of a solar streamer blowout coronal mass ejection arising from the streamer flank
Ruisheng Zheng, Yao Chen, and Bing Wang

TL;DR
This paper investigates the initiation mechanism of a specific type of streamer blowout CME originating from the streamer flank, highlighting the roles of external and internal magnetic reconnections observed during filament eruption.
Contribution
It provides detailed observational evidence of external and internal reconnections involved in the initiation of SBO CMEs from the streamer flank, a previously elusive process.
Findings
Filament exhibited gradual external reconnections during rise.
Internal reconnections formed new lower loops and Y-shaped structures.
External and internal reconnections are key to SBO CME initiation.
Abstract
Streamer blowout (SBO) coronal mass ejections (CMEs) represent a particular class of CMEs that are characterized by a gradual swelling of the overlying streamer and a slow CME containing a flux-rope structure. SBO CMEs arising from the streamer flank fall into a special category of SBO CMEs involving three lower arches under the higher streamer arcade. However, the initiation mechanism for this special category of SBO CMEs remains elusive, due to the observational limitations. Here we report critical observations of a SBO CME associated with the eruption of a polar crown filament that originated from the streamer flank. The filament slowly rose toward the solar equator with the writhing motion, and underwent a sudden acceleration before its eruption. Interestingly, during the rising, the filament fields experienced gradual external reconnections, which is evidenced by the dip-shaped…
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