Iron abundance in the solar photosphere. Application of a two-component model atmosphere
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20020656/pdf
Reference25 articles.
1. Fe i line shifts in the optical spectrum of the Sun
2. Chemical Abundances from Inversions of Stellar Spectra: Analysis of Solar‐Type Stars with Homogeneous and Static Model Atmospheres
3. A determination of the solar abundance of iron from the strong lines of Fe I
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