| Issue |
A&A
Volume 399, Number 2, February IV 2003
|
|
|---|---|---|
| Page(s) | 749 - 754 | |
| Section | The Sun | |
| DOI | https://doi.org/10.1051/0004-6361:20021820 | |
| Published online | 07 February 2003 | |
Evidence for a Flux Rope driven EUV wave and CME: Comparison with the Piston Shock Model
1
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, carl.foley@mssl.ucl.ac.uk
Received:
4
October
2002
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
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.