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Coronal heating
Authors:J. B. Zirker
Affiliation:(1) National Solar Observatory, National Optical Astronomy Observatories, 88349 Sunspot, NM, USA
Abstract:The prospects for observational tests of coronal heating theories are examined. Three heating mechanisms (Alfvén 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.Operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under cooperative agreement with the National Science Foundation.
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