Nov 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..148...43z&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 148, no. 1, p. 43-60
Physics
117
Direct Current, Heating, Magnetohydrodynamic Turbulence, Magnetohydrodynamic Waves, Photosphere, Solar Corona, Stellar Models, Convective Flow, Current Sheets, Field Aligned Currents, Magnetic Field Reconnection, Magnetic Relaxation, Plasma Density, Plasma Temperature, Solar Flares
Scientific paper
The prospects for observational tests of coronal heating theories are
examined. Three heating mechanisms (Alfven waves, D.C. electric
currents, and MHD turbulence) are reviewed from this point of view. Some
suggestions are offered for future tests but none, so far, would give
unambiguous critical results.
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