EAS Publications Series
Volume 44, 2010JENAM 2008: Grand Challenges in Computational Astrophysics
|Page(s)||101 - 105|
|Published online||20 January 2011|
H. Wozniak and G. Hensler (eds)
EAS Publications Series, 44 (2010) 101-105
Coronal EUV dimming – numerical simulations compared with SOHO observations
Astronomical Institute of Romanian Academy ; Romania
Our paper intends to estimate the EUV dimming appearing in a prominence eruption into a coronal mass ejection from the observationally point of few and so well from a numerical model. We have performed a numerical MHD simulation on a solar radius and obtained a CME originating from a prominence. The mass dimming was revealed clearly and we compared the mass evolution of the CME to that of an event observed on 14 January 2001 by SOHO.
© EAS, EDP Sciences 2011
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