Excitation of solar p-modes
文献类型：期刊论文
| 作者 | Bi SL(毕少兰) ; Li RF(李如凤)
|
| 刊名 | CHINESE ASTRONOMY AND ASTROPHYSICS
 |
| 出版日期 | 1998-04 |
| 卷号 | 22期号:2页码:205-214 |
| 关键词 | solar oscillation convective turbulence excitation mechanism |
| ISSN号 | 0275-1062 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Bi, SL |
| 英文摘要 | On the basis of a 5-dimensional, time/space separated description of convective turbulence and the mixing length theory we: calculated the excitation rate (E) over dot = E Gamma for a single solar p-mode. We found that (E) over dot varies as nu(7) or nu(-5) according as nu is below or above 3 mHz. Our result for the higher frequencies resolves a previous difficulty with the observations. It appears that solar p-modes are excited mainly by Reynolds stress fluctuations, rather than by entropy fluctuations. |
| 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] | TURBULENT CONVECTION ; GENERATION ; OSCILLATION ; SEISMOLOGY ; ENERGY ; STARS |
| 收录类别 | SCI |
| 原文出处 | http://www.sciencedirect.com/science/article/pii/S0275106298000290 |
| 语种 | 英语 |
| WOS记录号 | WOS:000082336500012 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/5144]  |
| 专题 | 云南天文台_恒星物理研究组 |
| 作者单位 | Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011 China |
| 推荐引用方式 GB/T 7714 | Bi SL,Li RF. Excitation of solar p-modes[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,1998,22(2):205-214. |
| APA | Bi SL,&Li RF.(1998).Excitation of solar p-modes.CHINESE ASTRONOMY AND ASTROPHYSICS,22(2),205-214. |
| MLA | Bi SL,et al."Excitation of solar p-modes".CHINESE ASTRONOMY AND ASTROPHYSICS 22.2(1998):205-214. |
入库方式： OAI收割
来源：云南天文台
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