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TURBULENT CONVECTION MODEL IN THE OVERSHOOTING REGION. I. EFFECTS OF THE CONVECTIVE MIXING IN THE SOLAR OVERSHOOTING REGION
Zhang QS(张钱生)1,2,3; Li Y(李焱)1,2; Zhang, QS (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, POB 110, Kunming 650011, Peoples R China.
发表期刊ASTROPHYSICAL JOURNAL
2012-02-10
卷号746期号:1
DOI10.1088/0004-637X/746/1/50
产权排序第1完成单位
收录类别SCI
关键词Convection Diffusion Sun: Helioseismology Sun: Interior Turbulence
摘要The overshooting in the framework of the turbulent convection model is investigated in the solar overshooting region. The overshooting mixing is treated as a diffusive process. It is found that the sound speed profile can be improved to be in good agreement with helioseismic inversions. The bump in the sound speed differences between solar models and the helioseismical inversions below the base of the solar convective envelope is almost eliminated by the overshooting mixing. The overshooting mixing leads to a significant depletion of Li in the main-sequence stage. Li abundance in the solar surface can be reduced to about 1% of its initial abundance in the solar models with the overshooting mixing. The solar model with the overshooting shows a smooth profile of the temperature gradient, which is also favored by the helioseismology.
项目资助者National Natural Science Foundation of China [10673030, 10973035] ; Science Foundation of Yunnan Observatory [Y0ZX011009]
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0004-637X
URL查看原文
归档日期2012-02-13
WOS记录号WOS:000302861300050
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]NONLOCAL CONVECTION ; CHEMICAL-COMPOSITION ; ELEMENT DIFFUSION ; ZONE ; ABUNDANCES ; HELIOSEISMOLOGY ; OPACITIES ; BASE ; ENVELOPE ; STARS
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被引频次:33[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/5224
专题恒星物理研究组
中国科学院天体结构与演化重点实验室
通讯作者Zhang, QS (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, POB 110, Kunming 650011, Peoples R China.
作者单位1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming 650011, China
2.Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
3.Graduate School of Chinese Academy of Sciences, Beijing 100039, China
第一作者单位中国科学院云南天文台
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GB/T 7714
Zhang QS,Li Y,Zhang, QS . TURBULENT CONVECTION MODEL IN THE OVERSHOOTING REGION. I. EFFECTS OF THE CONVECTIVE MIXING IN THE SOLAR OVERSHOOTING REGION[J]. ASTROPHYSICAL JOURNAL,2012,746(1).
APA Zhang QS,Li Y,&Zhang, QS .(2012).TURBULENT CONVECTION MODEL IN THE OVERSHOOTING REGION. I. EFFECTS OF THE CONVECTIVE MIXING IN THE SOLAR OVERSHOOTING REGION.ASTROPHYSICAL JOURNAL,746(1).
MLA Zhang QS,et al."TURBULENT CONVECTION MODEL IN THE OVERSHOOTING REGION. I. EFFECTS OF THE CONVECTIVE MIXING IN THE SOLAR OVERSHOOTING REGION".ASTROPHYSICAL JOURNAL 746.1(2012).
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