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Lithium depletion in the solar atmosphere
Xiong, DR; Deng, LC
AbstractUsing a complete non-local convection theory, we carried out the theoretical calculations of Li-7 depletion of the solar convective envelope models with different convective parameters c(1) and c(2), and got a model of the solar convection zone consistent with the observed Li-7 abundance and the depth of the solar convection zone determined by helioseismic techniques. The overshooting distance of effective non-local convective mixing of 7Li is very extensive, which is about 1.07Hp or 0.09R(circle dot). However, the super-radiative temperature zone is much narrower, and it is only 0.20Hp or 0.016R(circle dot).
KeywordLi-7 Abundance Convection Overshooting Solar Interior
Indexed BySCI
WOS IDWOS:000172661300003
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Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Affiliation1.Acad Sinica, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Xiong, DR,Deng, LC. Lithium depletion in the solar atmosphere[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2001,25(4):412-415.
APA Xiong, DR,&Deng, LC.(2001).Lithium depletion in the solar atmosphere.CHINESE ASTRONOMY AND ASTROPHYSICS,25(4),412-415.
MLA Xiong, DR,et al."Lithium depletion in the solar atmosphere".CHINESE ASTRONOMY AND ASTROPHYSICS 25.4(2001):412-415.
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