| Relations between solar radio millisecond spike-type III bursts in metric waves and acceleration processes of coronal electrons | |
Ma Y(马媛)1,3 ; Xie RX(谢瑞祥)1,3; Zheng XM(郑向明)1,2; Wang M(汪敏)1,3; Huang, GL2,3; Ma, Y (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China.
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| 发表期刊 | CHINESE ASTRONOMY AND ASTROPHYSICS
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| 2001-01 | |
| 卷号 | 25期号:1页码:111-119 |
| DOI | 10.1016/S0275-1062(01)00050-9 |
| 产权排序 | 第1完成单位 |
| 收录类别 | SCI |
| 关键词 | Solar Radio Burst Fine Structures Electron Acceleration |
| 摘要 | This paper presents a comprehensive account of the data obtained with the metric wave radio spectrograph of Yunnan Observatory during the maximum of 22nd solar activity cycle and some type III bursts of symbiotic millisecond class spikes discovered in the data reduction. The various morphologies reveal the relation between the occurrences of type III bursts and millisecond spikes. From an analysis of two typical events according to the time sequence of appearances of spikes and type III bursts as well as the characteristics of continuity and transformation in morphology, it is verified that the region of acceleration of coronal electrons is located above the sources of millisecond spikes and type III bursts. The authors' observations show that the interface frequency corresponding to type III bursts lies near 250 MHz. Finally, the authors attempt to interpret qualitatively the generation mechanism of the metric wave millisecond spike-type III bursts with the plasma hypothesis. |
| 语种 | 英语 |
| 学科领域 | Astronomy & Astrophysics |
| 文章类型 | Article |
| ISSN | 0275-1062 |
| URL | 查看原文 |
| WOS记录号 | WOS:000167510400014 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | EMISSION |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6047 |
| 专题 | 太阳物理研究组 |
| 通讯作者 | Ma, Y (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China. |
| 作者单位 | 1.Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011 China 2.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008 China 3.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 China |
| 第一作者单位 | 中国科学院云南天文台 |
| 推荐引用方式 GB/T 7714 | Ma Y,Xie RX,Zheng XM,et al. Relations between solar radio millisecond spike-type III bursts in metric waves and acceleration processes of coronal electrons[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2001,25(1):111-119. |
| APA | Ma Y,Xie RX,Zheng XM,Wang M,Huang, GL,&Ma, Y .(2001).Relations between solar radio millisecond spike-type III bursts in metric waves and acceleration processes of coronal electrons.CHINESE ASTRONOMY AND ASTROPHYSICS,25(1),111-119. |
| MLA | Ma Y,et al."Relations between solar radio millisecond spike-type III bursts in metric waves and acceleration processes of coronal electrons".CHINESE ASTRONOMY AND ASTROPHYSICS 25.1(2001):111-119. |
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