The calculation of theoretical chromospheric models and predicted OSO 1 spectra

Details The calculation of theoretical chromospheric models and predicted OSO 1 spectra The calculation of theoretical chromospheric models and predicted OSO 1 spectra

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sao..rept.....a&link_type=abstract

Progress Report, 1 Jul. 1974 - 31 Dec. 1975 Smithsonian Astrophysical Observatory, Cambridge, MA.

Other

Astronomical Models, Chromosphere, Photosphere, Solar Spectra, Chemical Composition, Oso-1, Solar Atmosphere, Spectrum Analysis

Scientific paper

Theoretical solar chromospheric and photospheric models are computed for use in analyzing OSO 8 spectra. The Vernazza, Avrett, and Loeser (1976) solar model is updated and self-consistent non-LTE number densities for H I, He I, He II, C I, Mg I, Al I, Si I, and H(-) are produced. These number densities are used in the calculation of a theoretical solar spectrum from 90 to 250 nm, including approximately 7000 lines in non-LTE. More than 60,000 lines of other elements are treated with approximate source functions.

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