Evidence for a flux rope driven EUV wave and CME: Comparison with the piston shock model

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Abstract

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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Foley, C. R., Harra, L. K., Matthews, S. A., Culhane, J. L., & Kitai, R. (2003). Evidence for a flux rope driven EUV wave and CME: Comparison with the piston shock model. Astronomy and Astrophysics, 399(2), 749–754. https://doi.org/10.1051/0004-6361:20021820

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