Turbulence and solar p-mode oscillations
文献类型：期刊论文
| 作者 | Bi SL(毕少兰) ; Xu HY(许华崟)
|
| 刊名 | ASTROPHYSICS AND SPACE SCIENCE
 |
| 出版日期 | 2002 |
| 卷号 | 279期号:3页码:191-202 |
| ISSN号 | 0004-640X |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Bi, SL (reprint author), Chinese Acad Sci, NAOCAS, Yunnan Observ, Kunming 650011, Peoples R China. |
| 英文摘要 | 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. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | FREQUENCIES ; EXCITATION ; CONVECTION ; SEISMOLOGY ; INTERIOR ; STRESS |
| 收录类别 | SCI |
| 原文出处 | http://link.springer.com/article/10.1023%2FA%3A1015136218125 |
| 语种 | 英语 |
| WOS记录号 | WOS:000174968900001 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/5160]  |
| 专题 | 云南天文台_恒星物理研究组 |
| 作者单位 | Yunnan Observatory, NAOCAS, Chinese Academy of Sciences, Kunming, 650011, P.R. China |
| 推荐引用方式 GB/T 7714 | Bi SL,Xu HY. Turbulence and solar p-mode oscillations[J]. ASTROPHYSICS AND SPACE SCIENCE,2002,279(3):191-202. |
| APA | Bi SL,&Xu HY.(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. |
入库方式： OAI收割
来源：云南天文台
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。