Solar Coronal Heating and Turbulence

Details Solar Coronal Heating and Turbulence Solar Coronal Heating and Turbulence

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf...95g&link_type=abstract

SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004. Edited by F. Combes, D. Barret

Astronomy and Astrophysics

Astrophysics

Scientific paper

It is now clearly established that the solar coronal heating is due to the presence of the magnetic field which is revealed for example through intermittent structures like X-ray bright points, at scales smaller than 10 arcsec, or solar flares at larger scales. The widely accepted scenario for the formation of such structures is the flaring of magnetic loops which would be the main heating source for the corona. In this talk a brief review will be given on observations and heating models of magnetic loops.

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