The Heating of Solar Coronal Loops by Alfvén Wave Turbulence
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/849/i=1/a=46/pdf
Reference192 articles.
1. TURBULENT DIFFUSION IN THE PHOTOSPHERE AS DERIVED FROM PHOTOSPHERIC BRIGHT POINT MOTION
2. Granulation, Magneto-Hydrodynamic Waves, and the Heating of the Solar Corona
3. OBSERVING THE FINE STRUCTURE OF LOOPS THROUGH HIGH-RESOLUTION SPECTROSCOPIC OBSERVATIONS OF CORONAL RAIN WITH THE CRISP INSTRUMENT AT THE SWEDISH SOLAR TELESCOPE
4. THE ROLE OF TORSIONAL ALFVÉN WAVES IN CORONAL HEATING
5. Predicting Observational Signatures of Coronal Heating by Alfvén Waves and Nanoflares
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