Fluxon modeling of breakout CMEs

Details Fluxon modeling of breakout CMEs Fluxon modeling of breakout CMEs

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh41b1675r&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SH41B-1675

Astronomy and Astrophysics

Astrophysics

[7509] Solar Physics, Astrophysics, And Astronomy / Corona, [7513] Solar Physics, Astrophysics, And Astronomy / Coronal Mass Ejections, [7526] Solar Physics, Astrophysics, And Astronomy / Magnetic Reconnection

Scientific paper

The pivotal element of the classic breakout model of CME initiation is reconnection that occurs above inner magnetic field sheared by rotation. We research this model with the FLUX code both with and without reconnection. Without reconnection an eruption occurs after several turns have been injected into the active region. The resultant expansion or eruption is more like a kink-unstable flux rope than a classic breakout CME. By varying whether and where reconnection is allowed, we determine the location of magnetic free energy release in the breakout model.

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