A solar continuum model

Details A solar continuum model A solar continuum model

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987acasn..28..336j&link_type=abstract

(Acta Astronomica Sinica, vol. 28, 1987, p. 336-344) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 12, June 1988, p.

Astronomy and Astrophysics

Astronomy

Continuum Modeling, Limb Darkening, Photosphere, Solar Spectra, Stellar Models, Infrared Astronomy, Visible Spectrum

Scientific paper

A model solar photosphere is derived from observed absolute intensity and limb darkening of the continuum spectrum between 4000 and 24018 A. The results, with lg tau(c) at 5000 A as argument, show good agreement between theoretical results and observations. For the limb darkening coefficient and the continuum absolute intensity of the center of the solar disk, the mean relative errors are 1.2 percent and 0.68 percent, respectively. Differences between the results obtained by this model and those from the Harvard-Smithsonian Reference Atmosphere model (Gingerich et al., 1971) are discussed.

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