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Tracking the Evolution of A Coherent Magnetic Flux Rope Continuously from the Inner to the Outer Corona
X. Cheng, M. D. Ding, Y. Guo +6
The magnetic flux rope (MFR) is believed to be the underlying magnetic structure of coronal mass ejections (CMEs). However, it remains unclear how an MFR evolves into and forms the…
A Study of Fast Flareless Coronal Mass Ejections
H. Q. Song, Y. Chen, D. D. Ye +5
Two major processes have been proposed to convert the coronal magnetic energy into the kinetic energy of a coronal mass ejection (CME): resistive magnetic reconnection and ideal ma…
Investigating Two Successive Flux Rope Eruptions In A Solar Active Region
X. Cheng, J. Zhang, M. D. Ding +4
We investigate two successive flux rope (FR1 and FR2) eruptions resulting in two coronal mass ejections (CMEs) on 2012 January 23. Both FRs appeared as an EUV channel structure in…
Topical Issue in Solar Physics: Flux-rope Structure of Coronal Mass Ejections Preface
N. Gopalswamy, T. Nieves-Chinchilla, M. Hidalgo +4
This Topical Issue of Solar Physics, devoted to the study of flux-rope structure in coronal mass ejections (CMEs), is based on two Coordinated Data Analysis Workshops (CDAWs) held…