中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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; Zhao, G
刊名ASTRONOMY & ASTROPHYSICS
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

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。