Alfvén Wave Turbulence as a Coronal Heating Mechanism: Simultaneously Predicting the Heating Rate and the Wave-induced Emission Line Broadening
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/845/i=2/a=98/pdf
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1. A MODEL FOR THE SOURCES OF THE SLOW SOLAR WIND
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3. Signatures of Alfvén waves in the polar coronal holes as seen by EIS/Hinode
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