Coronal EUV dimming – numerical simulations compared with SOHO observations

C. Dumitrache; M. Mierla

doi:10.1051/eas/1044017

All issues

Volume 44 (2010)

EAS Publications Series, 44 (2010) 101-105

Abstract

Issue		EAS Publications Series Volume 44, 2010 JENAM 2008: Grand Challenges in Computational Astrophysics


Page(s)		101 - 105
DOI		https://doi.org/10.1051/eas/1044017
Published online		20 January 2011

Grand Challenges in Computational Astrophysics
H. Wozniak and G. Hensler (eds)
EAS Publications Series, 44 (2010) 101-105

Coronal EUV dimming – numerical simulations compared with SOHO observations

C. Dumitrache and M. Mierla

Astronomical Institute of Romanian Academy ; Romania
e-mail: crisd@aira.astro.ro

Abstract

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.