On the Nature of the Three-part Structure of Solar Coronal Mass Ejections

Coronal mass ejections (CMEs) result from eruptions of magnetic flux ropes (MFRs) and can possess a three-part structure in white-light coronagraphs, including a bright front, dark cavity, and bright core. In traditional opinion, the bright front forms due to the plasma pileup along the MFR border,...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Hongqiang Song, Jie Zhang, Leping Li, Zihao Yang, Lidong Xia, Ruisheng Zheng, Yao Chen
Format:	Article
Language:	English
Published:	IOP Publishing 2022-01-01
Subjects:	Solar coronal mass ejections Solar activity Solar coronal loops Solar flares
Online Access:	https://doi.org/10.3847/1538-4357/aca6e0