Asymptotic analysis of linear non-adiabatic non-radial oscillation of the solar p-modes | |
Bi SL(毕少兰); Li RF(李如凤) | |
刊名 | ASTRONOMY & ASTROPHYSICS |
1997-01-20 | |
卷号 | 317期号:3页码:949-952 |
关键词 | solar oscillation |
ISSN号 | 0004-6361 |
通讯作者 | Bi, SL |
产权排序 | 第一完成单位 |
英文摘要 | The non-adiabatic frequencies of a standard solar model are discussed in this paper. The physics describing the radiative losses is included in the non-adiabatic effects. An asymptotic approximation to the non-adiabatic non-radial p-modes of the Sun is developed. An exact solution of non-adiabatic oscillations, which results in an eigenfrequency equation with the model-dependent surface phase shift, is assumed in the outmost layers, where the asymptotic description is invalid. For the lower degree modes, the phase shift is a function of frequency alone. Compared with an adiabatic approximation, the non-adiabatic approximation of the p-mode frequencies fills more of the gap between theory and observation. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | FREQUENCIES ; SEISMOLOGY ; DIFFUSION ; SUN |
收录类别 | SCI |
原文出处 | http://adsabs.harvard.edu/abs/1997A%26A...317..949B |
语种 | 英语 |
WOS记录号 | WOS:A1997WG16900040 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/5140] |
专题 | 云南天文台_恒星物理研究组 |
作者单位 | Yunnan Observatory, P.O.Box 110, Kunming, Yunnan 650011, P.R. China |
推荐引用方式 GB/T 7714 | Bi SL,Li RF. Asymptotic analysis of linear non-adiabatic non-radial oscillation of the solar p-modes[J]. ASTRONOMY & ASTROPHYSICS,1997,317(3):949-952. |
APA | Bi SL,&Li RF.(1997).Asymptotic analysis of linear non-adiabatic non-radial oscillation of the solar p-modes.ASTRONOMY & ASTROPHYSICS,317(3),949-952. |
MLA | Bi SL,et al."Asymptotic analysis of linear non-adiabatic non-radial oscillation of the solar p-modes".ASTRONOMY & ASTROPHYSICS 317.3(1997):949-952. |
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