MHD Simulation of Solar Coronal Mass Ejection

Details MHD Simulation of Solar Coronal Mass Ejection MHD Simulation of Solar Coronal Mass Ejection

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005padeu..15...45d&link_type=abstract

In: Proceedings of the British-Romanian-Hungarian N+N+N Workshop for Young Researchers on Plasma- and Astrophysics: from laborat

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Time dependent magnetohydrodynamic computations on three solar radii,
starting with a current sheet initial configuration, is presented. A
prominence formation and eruption, trigger CMEs in 'raffales', with a
coronal streamer formation as last result.

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