Turbulence and solar p-mode oscillations

doi:10.1023/A:1015136218125

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	Turbulence and solar p-mode oscillations
	Bi SL(毕少兰); Xu HY(许华崟); Bi, SL (reprint author), Chinese Acad Sci, NAOCAS, Yunnan Observ, Kunming 650011, Peoples R China.
发表期刊	ASTROPHYSICS AND SPACE SCIENCE
	2002
卷号	279 期号:3 页码:191-202
DOI	10.1023/A:1015136218125
产权排序	第1完成单位
收录类别	SCI
摘要	The discrepancy between observed and theoretical mode frequencies can be used to examine the reliability of the standard solar model as a faithful representation of solar real situation. With the help of an improved time-dependent convective model that takes into account contribution of the full spatial and temporal turbulent energy spectrum, we study the influence of turbulent pressure on structure and solar p-mode frequencies. For the radial modes we find that the Reynolds stress produces signification modifications in structure and p-mode spectrum. Compared with an adiabatic approximation, the discrepancy is largely removed by the turbulent correction.
语种	英语
学科领域	Astronomy & Astrophysics
文章类型	Article
ISSN	0004-640X
URL	查看原文
归档日期	2002-06-04
WOS记录号	WOS:000174968900001
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	FREQUENCIES ; EXCITATION ; CONVECTION ; SEISMOLOGY ; INTERIOR ; STRESS
引用统计	被引频次：3[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/114a53/5160
专题	恒星物理研究组
通讯作者	Bi, SL (reprint author), Chinese Acad Sci, NAOCAS, Yunnan Observ, Kunming 650011, Peoples R China.
作者单位	Yunnan Observatory, NAOCAS, Chinese Academy of Sciences, Kunming, 650011, P.R. China
第一作者单位	中国科学院云南天文台
推荐引用方式 GB/T 7714	Bi SL,Xu HY,Bi, SL . Turbulence and solar p-mode oscillations[J]. ASTROPHYSICS AND SPACE SCIENCE,2002,279(3):191-202.
APA	Bi SL,Xu HY,&Bi, SL .(2002).Turbulence and solar p-mode oscillations.ASTROPHYSICS AND SPACE SCIENCE,279(3),191-202.
MLA	Bi SL,et al."Turbulence and solar p-mode oscillations".ASTROPHYSICS AND SPACE SCIENCE 279.3(2002):191-202.

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文件名称/大小	文献类型	版本类型	开放类型	使用许可
Turbulence and Solar（98KB）	期刊论文	作者接受稿	开放获取	CC BY-NC-SA	浏览请求全文