A model of the solar transition region and corona for the minimum of activity

Details A model of the solar transition region and corona for the minimum of activity A model of the solar transition region and corona for the minimum of activity

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....48..367c&link_type=abstract

Astronomy and Astrophysics, vol. 48, no. 3, May 1976, p. 367-371.

Astronomy and Astrophysics

Astrophysics

1

Astronomical Models, Brightness Temperature, Solar Atmosphere, Solar Corona, Solar Radio Emission, Atmospheric Models, Atmospheric Stratification, Hydrostatics, Optical Thickness, Solar Activity Effects, Solar X-Rays, Ultraviolet Radiation

Scientific paper

Constant pressure and conductive flux in the transition region and constant temperature and hydrostatic equilibrium in the corona are assumed to allow the use of simple formulas to derive the brightness temperature. Contributions to the brightness temperature from the transition region and corona are compared. Three of the very few available observations in the relevant frequency range are used to deduce a model of these two regions for solar activity minima, which turns out to be quite similar to UV and X-ray models of coronal holes.

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