The solar corona and the solar wind

Details The solar corona and the solar wind The solar corona and the solar wind

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981nassp.450..135z&link_type=abstract

In NASA. Goddard Space Flight Center The Sun as a Star p 135-162 (SEE N81-27008 17-90)

Physics

19

Magnetic Variations, Periodic Variations, Solar Corona, Solar Magnetic Field, Solar Wind, Photosphere, Solar Atmosphere, Stellar Structure, Sun

Scientific paper

A stellar corona is an extended atmospheric region that is maintained at a significantly higher temperature than that of the stellar photosphere by nonthermal energy input. The solar corona stands as a prototype for all stellar coronas and is a prime example of a stellar atmosphere in which nonthermal processes predominate. Nonthermal processes are those in which the local flux of energy bears no direct relation to the internal energy of the gas or the quality of the radiation the gas emits and absorbs. Observations of the solar corona and the solar wind were surveyed and are presented.

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