The Birth of a Major Coronal Mass Ejection with Intricate Magnetic Structure from Multiple Active Regions

The Birth of a Major Coronal Mass Ejection with Intricate Magnetic Structure from Multiple Active Regions

Coronal mass ejections (CMEs) are the eruptions of magnetized plasma from the Sun and are considered the main driver of adverse space weather events. Hence, understanding their formation process, particularly the magnetic topology, is critical for accurate space weather prediction. Here, based on im...

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Bibliographic Details
Main Authors: J. H. Guo, Y. W. Ni, B. Schmieder, Y. Guo, C. Xia, P. Devi, R. Chandra, S. Poedts, R. Joshi, Y. H. Zhou, H. T. Li, P. F. Chen
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Magnetohydrodynamical simulations
Solar coronal mass ejections
Solar magnetic fields
Online Access:https://doi.org/10.3847/1538-4357/adb976
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https://doi.org/10.3847/1538-4357/adb976

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