Failure of a Solar Filament Eruption Caused by Magnetic Reconnection with Overlying Coronal Loops

Failure of a Solar Filament Eruption Caused by Magnetic Reconnection with Overlying Coronal Loops

The 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 a reconnection between an erupting filament and its overl...

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Bibliographic Details
Main Authors: 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, Yudi Ou
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar filament eruptions
Solar extreme ultraviolet emission
Solar corona
Plasma astrophysics
Solar flares
Solar magnetic reconnection
Online Access:https://doi.org/10.3847/1538-4357/ad9a56
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https://doi.org/10.3847/1538-4357/ad9a56

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