Abundance of iron in the solar atmosphere

Details Abundance of iron in the solar atmosphere Abundance of iron in the solar atmosphere

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...76b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, July-Aug. 1989, p. 76-80. In Russian.

Computer Science

Atmospheric Composition, Iron, Metallicity, Solar Atmosphere, Nonequilibrium Thermodynamics, Spectral Line Width, Thermodynamic Equilibrium

Scientific paper

The abundance of iron in the solar atmosphere calculated from Fe II lines exceeds that calculated from Fe I lines by at least 0.14 dex. As the excitation potential of Fe I lines increases, the iron abundance determined on the assumption of LTE also increases. It is concluded that the most likely value of iron abundance in the solar atmosphere is 7.8 dex.

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