Heating of the solar corona by the resonant absorption of Alfven waves

Details Heating of the solar corona by the resonant absorption of Alfven waves Heating of the solar corona by the resonant absorption of Alfven waves

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..445d&link_type=abstract

In its Coronal and Prominence Plasmas p 445-449 (SEE N87-20871 13-92)

Physics

2

Absorptivity, Heating, Magnetohydrodynamic Waves, Resonance, Solar Corona, Asymptotic Methods, Boundary Value Problems, Fourier Transformation, Mathematical Models, Plasmas (Physics)

Scientific paper

An improved method for calculating the resonance absorption heating rate is discussed and the results are compared with observations in the solar corona. The primary conclusion to be drawn from these calculations is that to the level of the approximation adopted, the observations of the heating rate and nonthermal line broadening in the solar corona are consistent with heating by the resonance absorption mechanism.

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