Simulation of dark lanes in post--flare supra--arcades

Using two simulations of 1.5D, for the first time, in Costa et al. (2009) and Shulz et al. (2010) we numerically reproduce the observational dark inflows described in Verwichte et al. (2005). We show that the dark tracks can be explained as hot plasma vacuums generated upstream of a slow magnetoacou...

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Bibliographic Details
Published inarXiv.org
Main Authors Maglione, L S, Schneiter, E M, Costa, A, Elaskar, S
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 18.01.2011
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