The Dynamic Evolutionary Processes of the Magnetic Fields in the Solar Active Region Boulder 5395
1993 ◽
Vol 141
◽
pp. 457-460
Keyword(s):
AbstractIn this paper, based on observational information we proposed an opening bipolar magnetic field model and studied numerically the dynamic evolutionary processes of the magnetic fields by solving a complete set of MHD equations. The aim is to discuss one of the mechanisms of energy build up of solar flares produced in the active region Boulder 5395.