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Coronal heating due to the emergence of magnetic flux
Authors:S T Wu  M T Song  C C Cheng  M Dryer
Institution:(1) Center for Space Plasma and Aeronomic Research and Department of Mechanical Engineering, The University of Alabama in Huntsville, 35899 Huntsville, AL, USA;(2) Naval Research Laboratory, 20375 Washington, DC, USA;(3) Space Environment Laboratory/ERL, National Oceanic and Atmospheric Administration, 80303 Boulder, CO, USA
Abstract:A self-consistent time-dependent, two-dimensional MHD model with a realistic energy equation is developed to understand the origin of bright coronal emission accompanying the occurrence of a new bipolar magnetic region. The motivation for this study is the interpretation of anticipated observations to be made by the SOHO mission.Purple Mt. Obser., PRC
Keywords:Coronal Heating
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