On the Nature of the Three-part Structure of Solar Coronal Mass Ejections
Hongqiang Song, Jie Zhang, Leping Li, Zihao Yang, Lidong Xia, Ruisheng, Zheng, and Yao Chen

TL;DR
This paper challenges traditional views on the three-part structure of CMEs, proposing a new explanation supported by observations and a survey, emphasizing its fundamental role in understanding CME physics.
Contribution
It introduces a novel interpretation of CME structures, supported by a detailed event analysis and a comprehensive survey, redefining the nature of the three-part CME appearance.
Findings
CME front originates from plasma pileup along magnetic arcades
The bright core is a hot-channel magnetic flux rope
The dark cavity is a low-density zone between the CME front and the MFR
Abstract
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 the traditional opinion, the bright front forms due to the plasma pileup along the MFR border, the cavity represents the cross section of the MFR, and the bright core corresponds to the erupted prominence. However, this explanation on the nature of the three-part structure is being challenged. In this paper, we report an intriguing event occurred on 2014 June 14 that was recorded by multiple space- and ground-based instruments seamlessly, clearly showing that the CME front originates from the plasma pileup along the magnetic arcades overlying the MFR, and the core corresponds to a hot-channel MFR. Thus the dark cavity is not an MFR, instead it is a low-density zone between the CME…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Geomagnetism and Paleomagnetism Studies
