A group of solar microwave type III bursts with reversed drift rates on Nov 4, 1997
文献类型：期刊论文
| 作者 | Huang, GL; Fu, QJ; Qin, ZH |
| 刊名 | ASTROPHYSICS AND SPACE SCIENCE
 |
| 出版日期 | 1999 |
| 卷号 | 266期号:3页码:389-398 |
| 关键词 | ELECTRON-BEAMS RADIO FLARE PULSATIONS |
| ISSN号 | 0004-640X |
| 英文摘要 | The most important feature of the microwave type III bursts on Nov. 4, 1997 is the periodically reversed drift rates, which may be contributed to a group of electron beams trapped by a huge magnetic tube (10(4) km). It is suggested that these electron beams are accelerated by the same mechanism, because there is a power law distribution with index 3.2 in the energetic spectrum of the beam. On the other hand, the energy release in each pulse is quasi-quantized, which is confirmed by the statistical correlation between the rising time and the burst flux. Both of these two results are based on the model of plasma instability responsible for the burst. |
| 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] | ELECTRON-BEAMS ; RADIO ; FLARE ; PULSATIONS |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000087108100004 |
| 公开日期 | 2013-02-01 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/8315]  |
| 专题 | 紫金山天文台_太阳活动的多波段观测研究团组 |
| 作者单位 | 1.Purple Mt Observ, Nanjing, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Beijing 100864, Peoples R China 3.Beijing Astron Observ, Beijing, Peoples R China 4.Nanjing Univ, Dept Astron, Nanjing, Peoples R China |
| 推荐引用方式 GB/T 7714 | Huang, GL,Fu, QJ,Qin, ZH. A group of solar microwave type III bursts with reversed drift rates on Nov 4, 1997[J]. ASTROPHYSICS AND SPACE SCIENCE,1999,266(3):389-398. |
| APA | Huang, GL,Fu, QJ,&Qin, ZH.(1999).A group of solar microwave type III bursts with reversed drift rates on Nov 4, 1997.ASTROPHYSICS AND SPACE SCIENCE,266(3),389-398. |
| MLA | Huang, GL,et al."A group of solar microwave type III bursts with reversed drift rates on Nov 4, 1997".ASTROPHYSICS AND SPACE SCIENCE 266.3(1999):389-398. |
入库方式： OAI收割
来源：紫金山天文台
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