Expansion-induced Three-part Morphology of the 2021 December 4 Coronal Mass Ejection

The typical structure of a coronal mass ejection (CME) was identified as a three-part morphology, which includes a bright front, a dark cavity, and a bright core, with the cavity and the core generally regarded as flux rope and eruptive prominence. However, there are three-part CMEs that are not ass...

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Главные авторы:	Liping Yang, Xueshang Feng, Fang Shen, Ming Xiong, Chenglong Shen, Yutian Chi, Yuming Wang, Kuo Yan, Mengxuan Ma, Yufen Zhou, Man Zhang, Xinhua Zhao
Формат:	Artigo
Язык:	Inglês
Опубликовано:	IOP Publishing 2025-01-01
Серии:	The Astrophysical Journal
Предметы:	Solar coronal mass ejections Solar wind Magnetohydrodynamics
Online-ссылка:	https://doi.org/10.3847/1538-4357/adb313
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