The solar corona and the origin of the solar wind

Details The solar corona and the origin of the solar wind The solar corona and the origin of the solar wind

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48..561c&link_type=abstract

(Advanced School of Astronomy, Course on the Sun, a Tool for Stellar Physics, 6th, Erice, Italy, Aug. 8-21, 1976.) Società Astro

Physics

Atmospheric Heating, Solar Atmosphere, Solar Corona, Solar Physics, Solar Wind, Chromosphere, Solar Protons, Stellar Models, Thermal Plasmas, Thermodynamic Properties

Scientific paper

The paper deals with the properties of the solar corona and the techniques by which they have been observed. The corona is treated, in general, as a spherically symmetric stationary gas. This model, although admittedly unrealistic, has a certain right to exist if it is considered as an average model (corresponding to a lower resolution or to a greater distance to the sun). Particular attention is given to the problem of coronal heating and to the solar wind.

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