The Impulsive Acceleration of a Solar Filament Eruption Associated with a B-class Flare

The Impulsive Acceleration of a Solar Filament Eruption Associated with a B-class Flare

The eruption of magnetic flux ropes (MFRs), often taking filaments together, leads to coronal mass ejections (CMEs). Theoretical studies propose that both the resistive magnetic reconnection and the ideal instability of an MFR system can release magnetic-free energy and accelerate CMEs (i.e., MFRs o...

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Bibliographic Details
Main Authors: Xinyue Wang, Hongqiang Song, Yao Chen, Leping Li, Zhenyong Hou, Ruisheng Zheng
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Solar filament eruptions
Solar activity
Solar flares
Online Access:https://doi.org/10.3847/1538-4357/acff5d

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