The resistive MHD equations are numerically solved in two dimensions for an initial-boundary-value problem which simulates reconnection between an emerging magnetic flux region and an overlying coronal magnetic field. The solution involves both ideal-MHD and resistive-MHD processes, and the solution shows an evolution which is remarkably suggestive of the preflare, impulsive, and main phases of the flare-cycle.
Numerical simulation of reconnection in an emerging magnetic flux region
Advances in Space Research ; 4 , 7 19
1984-01-01
Miscellaneous
No indication
English
Numerical simulation of reconnection in an emerging magnetic flux region
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