Predicting Coronal Emissions with Multiple Heating Rates

Physics

Scientific paper

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7509 Corona, 7524 Magnetic Fields

Scientific paper

A variety of proposed coronal heating mechanisms remain prominent in the literature, with insufficient observational constraints to distinguish between them. In an attempt to add further constraints, we create predicted coronal emission maps of several active regions using simple parametrizations of differing theoretical heating mechanisms and compare the results to the observed coronal emissions. The results are interpolated to a 3-d grid, convolved with instrument response function, and integrated over line of sight to simulate satellite observation of the modeled loops. We also discuss those factors which dominate the differences in observed and predicted coronal emission.

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