Deciphering the Slow-rise Precursor of a Major Coronal Mass Ejection

Coronal mass ejections are explosive plasma phenomena prevalently occurring on the Sun and probably on other magnetically active stars. However, how their pre-eruptive configuration evolves toward the main explosion remains elusive. Here, based on comprehensive observations of a long-duration precur...

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Bibliographic Details
Main Authors: X. Cheng, C. Xing, G. Aulanier, S. K. Solanki, H. Peter, M. D. Ding
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Letters
Subjects:
Online Access:https://doi.org/10.3847/2041-8213/acf3e4