Volume 399, Number 2, February IV 2003
|Page(s)||749 - 754|
|Published online||07 February 2003|
Evidence for a Flux Rope driven EUV wave and CME: Comparison with the Piston Shock Model
Mullard Space Science Laboratory, Department of Space and Climate Physics, Holmbury St Mary, Dorking, Surrey, RH5 6NT, UK
2 Kwasan and Hida Observatories, Kyoto University, Yamashina, Kyoto 607-8471, Japan
Corresponding author: C. Foley, firstname.lastname@example.org
Accepted: 5 December 2002
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).
Key words: Sun: coronal mass ejections (CMEs) / Sun: corona / Sun: filaments
© ESO, 2003
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