How Reconnection-unfavored Magnetic Flux Emergence Suppresses Solar Filament Eruptions

How Reconnection-unfavored Magnetic Flux Emergence Suppresses Solar Filament Eruptions

Magnetic flux emergence is traditionally considered to be a key trigger of solar filament eruptions, yet its role in suppressing filament eruptions remains less understood. Using multiwavelength observations from the Solar Dynamics Observatory, this study investigates a unique case of flux emergence...

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Bibliographic Details
Main Authors: Chengrui Zhou, Yuandeng Shen, Chun Xia, Hao Liang, Zehao Tang, Dongxu Liu, Surui Yao
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
Subjects:
Solar activity
Solar filaments
Solar chromosphere
Solar magnetic fields
Online Access:https://doi.org/10.3847/2041-8213/ade051
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