Heating of the solar corona

Details Heating of the solar corona Heating of the solar corona

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sf2a.conf..529b&link_type=abstract

SF2A-2006: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: D. Barret, F. Casoli, G.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The mechanisms of transport and dissipation of energy in the corona are the subject of a long-lasting controversy in solar physics, with implications on Solar-Terrestrial physics. I review some classical models of wave or current dissipation, and I discuss the role of turbulence, how it can help providing the small scales at which dissipation is more efficient, what observational and computational difficulties arise, what is being done to overcome them, and what new challenges we meet.

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