Magnetohydrodynamics (MHD) modelling of flare energy buildup, the energy release phase, and its propagation into heliospheric spaceSolar flare energy buildup at the photospheric level and energy release and transport into heliospheric space are examined using a composite MHD model. A four phase composite MHD model is described. An example demonstrating the applicability of the model is presented; the model was applied to the active region AR 2372. The limitations of this composite MHD model approach to analyzing solar flare energy buildup are discussed.
Document ID
19880023712
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Wu, S. T. (Alabama Univ. Huntsville, AL, United States)
Panitchob, S. (Alabama, University Huntsville, United States)