Models of material ejection

Details Models of material ejection Models of material ejection

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990stia...9350507s&link_type=abstract

Flares 22, Workshop, Chantilly, France, Oct. 1990, Paper, 14 p.

Physics

Astronomical Models, Solar Corona, Solar Flares, Solar Physics, Solar Prominences, Stellar Mass Ejection, Coronal Loops, Magnetic Field Configurations, Solar Magnetic Field, Thermal Energy

Scientific paper

Some recently developed models related to the formation of a coronal mass ejection (CME) are reviewed. The models individually consider the stability of a prominence, the eruption of a coupled prominence and CME configuration with driven reconnection below the prominence, magnetic arcade equilibrium, and coronal evolution due to shear motion. No effort is made to critique the various models. Their relevance to actual observed material ejections will ultimately be determined by detailed comparison with present and future observations.

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