This paper examines the relationship between a coronal wave, filament eruption, flare and Coronal Mass Ejection (CME) which occurred on 2001, April 10th. We study the pre-flare activity which includes the eruption of a filament and a coronal wave. A large X-ray flare and a CME follow. We discuss how these phenomena are related and compare our results to recent models. These are found to be largely consistent with the numerical simulations of a flux rope driven CME as presented recently in Chen et al. (2002)
International audienceCMEs have been observed for over 30 years with a wide variety of instruments. ...
International audienceCMEs have been observed for over 30 years with a wide variety of instruments. ...
We investigate the initiation and formation of Coronal Mass Ejections (CMEs) via a detailed two-view...
Two major coronal mass ejections (CMEs) observed during the Whole Heliosphere Interval (WHI) are com...
Abstract. Current theoretical ideas on the internal structure of CMEs suggest that a flux rope is ce...
Abstract We intend to provide a comprehensive answer to the question on whether all Coronal Mass Eje...
Abstract. We report on a complex study of a typical large W-limb CME event occurring on December 2, ...
Solar filament eruptions play a crucial role in triggering coronal mass ejections (CMEs). More than ...
On August 14, 2010 a wide-angled coronal mass ejection (CME) was observed. This solar eruption origi...
Coronal mass ejections (CMEs) are one of the primary manifestations of solar activity and can drive ...
Coronal mass ejections (CMEs) are the largest-scale eruptive phenomenon in the solar system, expandi...
11 pages, 9 figuresAims. Coronal mass ejections or CMEs are large dynamical solar-corona events. The...
International audienceCMEs have been observed for over 30 years with a wide variety of instruments. ...
International audienceCMEs have been observed for over 30 years with a wide variety of instruments. ...
On August 14, 2010 a wide-angled coronal mass ejection (CME) was observed. This solar eruption origi...
International audienceCMEs have been observed for over 30 years with a wide variety of instruments. ...
International audienceCMEs have been observed for over 30 years with a wide variety of instruments. ...
We investigate the initiation and formation of Coronal Mass Ejections (CMEs) via a detailed two-view...
Two major coronal mass ejections (CMEs) observed during the Whole Heliosphere Interval (WHI) are com...
Abstract. Current theoretical ideas on the internal structure of CMEs suggest that a flux rope is ce...
Abstract We intend to provide a comprehensive answer to the question on whether all Coronal Mass Eje...
Abstract. We report on a complex study of a typical large W-limb CME event occurring on December 2, ...
Solar filament eruptions play a crucial role in triggering coronal mass ejections (CMEs). More than ...
On August 14, 2010 a wide-angled coronal mass ejection (CME) was observed. This solar eruption origi...
Coronal mass ejections (CMEs) are one of the primary manifestations of solar activity and can drive ...
Coronal mass ejections (CMEs) are the largest-scale eruptive phenomenon in the solar system, expandi...
11 pages, 9 figuresAims. Coronal mass ejections or CMEs are large dynamical solar-corona events. The...
International audienceCMEs have been observed for over 30 years with a wide variety of instruments. ...
International audienceCMEs have been observed for over 30 years with a wide variety of instruments. ...
On August 14, 2010 a wide-angled coronal mass ejection (CME) was observed. This solar eruption origi...
International audienceCMEs have been observed for over 30 years with a wide variety of instruments. ...
International audienceCMEs have been observed for over 30 years with a wide variety of instruments. ...
We investigate the initiation and formation of Coronal Mass Ejections (CMEs) via a detailed two-view...