Failure of a solar filament eruption caused by magnetic reconnection with overlying coronal loops
Leping Li, Hongqiang Song, Yijun Hou, Guiping Zhou, Baolin Tan, Kaifan, Ji, Yongyuan Xiang, Zhenyong Hou, Yang Guo, Ye Qiu, Yingna Su, Haisheng Ji,, Qingmin Zhang, and Yudi Ou

TL;DR
This study presents observational evidence of magnetic reconnection between an erupting solar filament and overlying coronal loops, leading to a failed eruption, which enhances understanding of solar eruption dynamics.
Contribution
First direct observation of filament reconnection with overlying loops causing eruption failure, confirming theoretical models with detailed temperature and plasma flow analysis.
Findings
Reconnection occurred between filament and overlying loops.
Failed eruption associated with heating and formation of new loops.
Presence of plasmoid instability during the event.
Abstract
Failure of a filament eruption caused by magnetic reconnection between the erupting filament and the overlying magnetic field has been previously proposed in numerical simulations. It is, however, rarely observed. In this study, we report the reconnection between an erupting filament and its overlying coronal loops, that results in the failure of the filament eruption. On 2023 September 24, a filament was located in active region 13445. It slowly rose, quickly erupted, rapidly decelerated, and finally stopped, with an untwisting motion. As a failed eruption, the event is associated with an M4.4 flare but no coronal mass ejection. During the eruption, the filament became bright, and the overlying loops appeared first in the high-temperature channels. They have average temperatures of ~12.8 and ~9.6MK, respectively, indicating that both of them were heated. Two sets of new loops,…
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Taxonomy
TopicsSolar and Space Plasma Dynamics
