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Published online by Cambridge University Press: 20 January 2011
Our paper intends to estimate the EUV dimming appearing in a prominence eruption into acoronal mass ejection from the observationally point of few and so well from a numericalmodel. We have performed a numerical MHD simulation on a solar radius and obtained a CMEoriginating from a prominence. The mass dimming was revealed clearly and we compared themass evolution of the CME to that of an event observed on 14 January 2001 by SOHO.