A numerical simulation of an asymmetric breakout model for CMEs

Details A numerical simulation of an asymmetric breakout model for CMEs A numerical simulation of an asymmetric breakout model for CMEs

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsh52a..04m&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH52A-04

Physics

7513 Coronal Mass Ejections (2101), 2101 Coronal Mass Ejections (7513)

Scientific paper

We made a high resolution numerical simulation on an asymmetric 'magnetic breakout' model for CMEs. A fast CME was generated. The dynamics of the system is controlled by two reconnection events, i.e. the breakout reconnection at the outer x-point and the flare reconnection at the newly formed inner x-point. The CME is triggered by the former event and is accelerated by the latter event.

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