A type IV radio burst associated with type III burst, pulsation and spike emissions
文献类型：期刊论文
| 作者 | Wang M(汪敏)1 ; Xie RX(谢瑞祥)1; Duan ZC(段长春)1; Yan, YH2; Sych, RA3; Altyntsev, AT3
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| 刊名 | SOLAR PHYSICS
 |
| 出版日期 | 2003-02 |
| 卷号 | 212期号:2页码:407-424 |
| ISSN号 | 0038-0938 |
| 通讯作者 | Wang, M (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China. |
| 产权排序 | 第一完成单位 |
| 英文摘要 | A type IV radio burst accompanied by several normal- and reverse-drifting type III bursts, multiple long-term quasi-periodic pulsations and spikes was observed with the radio spectrometers (1.0-2.0 and 2.6-3.8 GHz) at National Astronomical Observatories of China (NAOC) on 23 September 1998. In combination with the images of Siberian Solar Radio Telescope (SSRT) of Russia, the complex and multiple magnetic structures inferred from the radio bursts reveal the existence of both large-scale and small-scale magnetic structures. This event suggests that the geometries of coronal magnetic fields contain multiple discrete electron acceleration/injection sites at different heights, and extended open and closed magnetic field lines. It can be shown that the energetic electrons gain access to open, diverging and closed field lines thus producing different types of radio bursts. From the characteristics of position, polarization, dispersion and displacement of the sources, the model of the type IV event is supported, which involves synchrotron emission from the electrons confined by the rapid scattering through the interaction of hydromagnetic wave with particles. |
| 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-BEAMS ; SOLAR ; CORONA ; FLARES ; TIMES ; FIELD ; VLA |
| 收录类别 | SCI |
| 原文出处 | http://link.springer.com/article/10.1023%2FA%3A1022929227798 |
| 语种 | 英语 |
| WOS记录号 | WOS:000181818600012 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/5611]  |
| 专题 | 云南天文台_射电天文研究组 |
| 作者单位 | 1.Yunnan Observatory, National Astronomical Observatories, Chinese Academy of Sciences, Kunming, 650011, China 2.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China 3.Institute of Solar-Terrestrial Physics, 126, Lermontov St., Irkutsk, 664033, Russia |
| 推荐引用方式 GB/T 7714 | Wang M,Xie RX,Duan ZC,et al. A type IV radio burst associated with type III burst, pulsation and spike emissions[J]. SOLAR PHYSICS,2003,212(2):407-424. |
| APA | Wang M,Xie RX,Duan ZC,Yan, YH,Sych, RA,&Altyntsev, AT.(2003).A type IV radio burst associated with type III burst, pulsation and spike emissions.SOLAR PHYSICS,212(2),407-424. |
| MLA | Wang M,et al."A type IV radio burst associated with type III burst, pulsation and spike emissions".SOLAR PHYSICS 212.2(2003):407-424. |
入库方式： OAI收割
来源：云南天文台
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