NLTE analysis of the solar potassium abundance
文献类型:期刊论文
作者 | Zhang, HW; Butler, K; Gehren, T; Shi, JR![]() ![]() |
刊名 | ASTRONOMY & ASTROPHYSICS
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出版日期 | 2006-07-01 |
卷号 | 453期号:2页码:723-727 |
关键词 | line : formation line : profiles Sun : abundances |
英文摘要 | 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. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000238322500035 |
源URL | [http://ir.bao.ac.cn/handle/114a11/7079] ![]() |
专题 | 国家天文台_光学天文研究部 |
作者单位 | 1.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China 2.Univ Munich, Inst Astron & Astophys, D-81679 Munich, Germany 3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Zhang, HW,Butler, K,Gehren, T,et al. NLTE analysis of the solar potassium abundance[J]. ASTRONOMY & ASTROPHYSICS,2006,453(2):723-727. |
APA | Zhang, HW,Butler, K,Gehren, T,Shi, JR,&Zhao, G.(2006).NLTE analysis of the solar potassium abundance.ASTRONOMY & ASTROPHYSICS,453(2),723-727. |
MLA | Zhang, HW,et al."NLTE analysis of the solar potassium abundance".ASTRONOMY & ASTROPHYSICS 453.2(2006):723-727. |
入库方式: OAI收割
来源:国家天文台
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