Theory of Coronal Mass Ejections [PDF]
Coronal mass ejections (CMEs) are extremely important phenomena, both for understanding the evolution of the global corona and for understanding and predicting space weather. Despite this importance, the physical explanation of CMEs remains largely confused.
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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 ...
Liping Yang+11 more
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Location of the activity responsible for the appearance of coronal mass ejections and the sites of their ejection from the solar surface [PDF]
N. S. Shilova
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Properties of coronal mass ejections: SOHO LASCO observations from January 1996 to June 1998 [PDF]
O. C. St. Cyr+13 more
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Time-dependent Hinode/EIS Atlas of a Coronal Mass Ejection Containing Cool Material
We report the first time-dependent spectral atlas of a coronal mass ejection (CME) observed by the Hinode/Extreme Ultraviolet Imaging Spectrometer (EIS).
E. M. Wraback+2 more
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Three‐dimensional and twisted: An MHD interpretation of on‐disk observational characteristics of coronal mass ejections [PDF]
S. E. Gibson, B. C. Low
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Change in photospheric magnetic flux during coronal mass ejections [PDF]
A. Lara, N. Gopalswamy, C. E. DeForest
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Editorial: Magnetic Flux Ropes: From the Sun to the Earth and Beyond
Rui Liu+6 more
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We report on the onset of a coronal mass ejection (CME) using spectroscopic observations in the 5303 Å coronal emission line with the Visible Emission Line Coronagraph (VELC) onboard ADITYA-L1, the recently launched first Indian space solar mission.
R. Ramesh+5 more
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The simulation of the coronal mass ejection‐shock system in the inner corona [PDF]
Beichen Zhang, Jingfang Wang
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