Abundances in solar atmosphere (Boyarchuk+, 1998)

Details Abundances in solar atmosphere (Boyarchuk+, 1998) Abundances in solar atmosphere (Boyarchuk+, 1998)

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ycat..80750586b&link_type=abstract

VizieR On-line Data Catalog: J/AZh/75/586. Originally published in: 1998AZh....75..586B; 1998ARep...42..517B

Computer Science

Sun, Spectroscopy, Abundances

Scientific paper

An analysis of the chemical composition of the solar atmosphere is performed using spectrograms of the daylight sky obtained on the ZTS telescope (dispersion 3Å/mm, signal-to-noise ration, S/N>100). The chemical composition derived in the framework of a Holweger-Muller atmosphere model are in excellent agreement with the generally accepted values. Analysis based on the models of Bell et al. (1976A&AS...23...37B) and Kurucz (1992RMxAA..23..181K) with Teff=5770K and logg=4.44 failed to give satisfactory results. (2 data files).

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