期刊
ASTRONOMY & ASTROPHYSICS
卷 453, 期 2, 页码 723-727出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20065074
关键词
line : formation; line : profiles; Sun : abundances
We investigate the formation of neutral potassium lines in the solar photosphere based on extensive statistical equilibrium calculations to determine the solar potassium abundance. The computations are based on a 68-level potassium atomic model. Hydrogen collisions were supplied with an enhancement factor S-H = 0.05 to the classical Drawin formula. Synthetic line profiles calculated from the level populations according to the NLTE departure coefficients were compared with the observed solar spectral atlas. The solar potassium abundance based on theoretical model atmospheres is log epsilon(circle dot) (K) = 5.12 +/- 0.03, which agrees with the meteoritic value of 5.09 +/- 0.05 compiled by Lodders.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据