On the nonlinear statistical relation of solar radio spikes | |
Wang, DY1; Li, DY2; Fu, QJ3; Xia ZG(夏志国)4 | |
刊名 | ASTROPHYSICS AND SPACE SCIENCE
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1997 | |
卷号 | 246期号:1页码:129-140 |
ISSN号 | 0004-640X |
通讯作者 | Wang, DY |
产权排序 | 第四完成单位 |
英文摘要 | Based on a modulation model of nonlinear parametric instability, some theoretical expectation of statistical relation of solar radio spikes have been obtained, It is shown that the modulation amplitude of spikes Delta S is approximately equal to the coherent flux of spikes S-c, excited by the electron cyclotron maser (ECM) instability; the repetition rate of spikes R is proportional to the square root of S-c; and the spikes phenomena can only display in the coherent emission with narrow frequency band. These theoretical expectation are consistent qualitatively with the present statistical relation and observational result of solar radio spikes. |
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] | ELECTRON-CYCLOTRON MASER ; X-RAY-EMISSION ; MILLISECOND SPIKES ; BURSTS ; INSTABILITIES ; SATURATION |
收录类别 | SCI |
原文出处 | http://link.springer.com/article/10.1007%2FBF00637404 |
语种 | 英语 |
WOS记录号 | WOS:A1997XL08600011 |
公开日期 | 2016-05-03 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/6888] ![]() |
专题 | 云南天文台_星系研究组 |
作者单位 | 1.Purple Mountain Observatory, 210008, Nanjing, China 2.East China Institute of Shipbuilding, 212003, Zhenjiang, China 3.Beijing Astronomical Observatory, 100080, Beijing, China 4.Yunnan Observatory, 650000, Kunming, China |
推荐引用方式 GB/T 7714 | Wang, DY,Li, DY,Fu, QJ,et al. On the nonlinear statistical relation of solar radio spikes[J]. ASTROPHYSICS AND SPACE SCIENCE,1997,246(1):129-140. |
APA | Wang, DY,Li, DY,Fu, QJ,&Xia ZG.(1997).On the nonlinear statistical relation of solar radio spikes.ASTROPHYSICS AND SPACE SCIENCE,246(1),129-140. |
MLA | Wang, DY,et al."On the nonlinear statistical relation of solar radio spikes".ASTROPHYSICS AND SPACE SCIENCE 246.1(1997):129-140. |
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