The heating of coronae

Details The heating of coronae The heating of coronae

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph..100..289i&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 100, Oct. 1985, p. 289-308.

Physics

54

Atmospheric Heating, Electrodynamics, Plasma Heating, Solar Corona, Stellar Models, Convection Currents, Coronal Loops, Coupling Coefficients, Energy Dissipation, Solar Radiation, Stellar Coronas, Stellar Magnetic Fields

Scientific paper

The electrodynamic model of coronas is examined as the essential link connecting X-ray observations to the basic mechanical properties of, for example, a star. Probably the most significant breakthroughs in understanding the heating of coronas have emerged from a global electrodynamics approach. Although this approach ties together a.c. (resonant) and d.c. (non-resonant) heating mechanisms, the detailed physics of the dissipation process is still not clearly understood.

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