New models of solar faculae

Details New models of solar faculae New models of solar faculae

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...232..923c&link_type=abstract

Astrophysical Journal, Part 1, vol. 232, Sept. 15, 1979, p. 923-928. Research supported by the Aerospace Corp.;

Astronomy and Astrophysics

Astrophysics

56

Atmospheric Models, Faculae, Solar Atmosphere, Solar Magnetic Field, Field Strength, Optical Thickness, Photosphere, Pressure Effects, Temperature Gradients, Time Dependence

Scientific paper

A new semiempirical model of photospheric faculae is presented in tabular form. The magnetic field is estimated from horizontal pressure equilibrium without tension forces. The geometry of the flux tube is determined from this estimated magnetic field and an assumed flux of 4.4 x 10 to the 17th gauss sq cm. The model is discussed in relation to recent observations.

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