Physics
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp14a..02l&link_type=abstract
American Geophysical Union, Spring Meeting 2005, abstract #SP14A-02
Physics
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.
Fisher George H.
Leka Kimberly Dawn
Lundquist Loraine L.
McTiernan James M.
Metcalf Thomas R.
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