Early Evolution of the Cavity and Core of a Coronal Mass Ejection in the Inner Corona
Shuting Li, Li Feng, Beili Ying, Hongqiang Song, Guanglu Shi, Jiahui Shan, Jie Zhao, Weiqun Gan

TL;DR
This study uses seamless inner corona observations to reveal the early evolution of a CME's cavity and core, showing temperature and speed changes that support the magnetic flux rope model of CME structure.
Contribution
It provides new insights into the early development of CME components, especially the temperature and kinematic evolution of the cavity and core, supporting the magnetic flux rope interpretation.
Findings
CME cavity is cooler than the prominence and fills with bright loop-like structures.
The core undergoes slow-rise, fast-rise, and residual acceleration phases.
The cavity lags behind the core by about 4 minutes and has lower peak speed.
Abstract
Coronal mass ejections (CMEs) typically exhibit a three-component structure in white-light (WL) coronagraphs. Utilizing the seamless observations of the inner corona ( 3 R), we have revealed the early evolution of the cavity and core of a CME starting at 18:20 UT on 2014 October 14. The CME originates from a hot channel (HC), which appears as the bright core and compresses the cavity in WL images. Specifically, most of the dark cavity in WL is filled by bright loop-like structures in 174 \AA. The differential emission measure (DEM) analysis indicates that the electron temperature decreases from the core (13.4 MK) to the cavity (1.35 MK), and the CME cavity is significantly cooler than that enshrouding a prominence ( 2 MK). The effective temperature of the cavity increases over time in general, probably due to the compression by the HC expansion. The…
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Taxonomy
TopicsSolar and Space Plasma Dynamics
