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The Dynamic Evolutionary Processes of the Magnetic Fields in the Solar Active Region Boulder 5395
Published online by Cambridge University Press: 12 April 2016
Abstract
In 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.
- Type
- Session 7. Magnetic Shear and Electric Currents
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- Copyright © Astronomical Society of the Pacific 1993