A Self-consistent Model of the Coronal Heating and Solar Wind Acceleration Including Compressible and Incompressible Heating Processes
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/853/i=2/a=190/pdf
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1. Granulation, Magneto-Hydrodynamic Waves, and the Heating of the Solar Corona
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