Evidence for a Flux Rope driven EUV wave and CME: Comparison with the Piston Shock Model

Details Evidence for a Flux Rope driven EUV wave and CME: Comparison with the Piston Shock Model Evidence for a Flux Rope driven EUV wave and CME: Comparison with the Piston Shock Model

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26a...399..749f&link_type=abstract

Astronomy and Astrophysics, v.399, p.749-754 (2003)

Astronomy and Astrophysics

Astrophysics

9

Sun: Coronal Mass Ejections (Cmes), Sun: Corona, Sun: Filaments

Scientific paper

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).

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