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Numerical Modeling of Coronal Mass Ejections Based on Various Pre-Event Model Atmospheres
DOI: 10.1007/BF00732075 Bibcode: 1995SoPh..161..365W

Wu, S. T.; Poletto, G.; Suess, S. T. +1 more

We examine how the initial state (pre-event corona) affects the numerical MHD simulation for a coronal mass ejection (CME). Earlier simulations based on a pre-event corona with a homogeneous density and temperature distribution at the lower boundary (i.e., solar surface) have been used to analyze the role of streamer properties in determining the …

1995 Solar Physics
Ulysses 29