Occurrence of bidirectional type III bursts in solar flares
文献类型：期刊论文
| 作者 | Ma, Y.1 ; Wang, De Yu2; Xie, R. X.1; Wang, M.1; Yan, Y. H.3
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| 刊名 | ASTROPHYSICS AND SPACE SCIENCE
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| 出版日期 | 2008-11-01 |
| 卷号 | 318期号:1-2页码:87-92 |
| 关键词 | Solar radio emission Type III burst Solar activity |
| 英文摘要 | The 13 pairs of type III bursts with the bidirectional drift structures recorded with the spectrograph in the frequency ranges of 230-300 MHz and 625-1500 MHz at the Yunnan Observatory and 2600-3800 MHz at the Beijing National Astronomical Observatories are analyzed in this present article and the outstanding characteristics of these events are obtained. These bursts respectively reveal that the separatrix frequency between the bursts with positive and negative drifts comes between 250 MHz and 3420 MHz, with a gap being between 0.6 MHz and 110 MHz; the duration is 53 ms-1880 ms and the frequency drift rate is between 45 MHz/s and 56000 MHz/s. The drift rate at metric wavelengths is relatively low, only a few decades of MHz while it is comparatively high at microwave wavelengths, reaching 56000 MHz/s. The qualitative explanation of these events is given in this paper. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000261185500011 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/8366]  |
| 专题 | 国家天文台_应用天文研究部 |
| 作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China 2.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
| 推荐引用方式 GB/T 7714 | Ma, Y.,Wang, De Yu,Xie, R. X.,et al. Occurrence of bidirectional type III bursts in solar flares[J]. ASTROPHYSICS AND SPACE SCIENCE,2008,318(1-2):87-92. |
| APA | Ma, Y.,Wang, De Yu,Xie, R. X.,Wang, M.,&Yan, Y. H..(2008).Occurrence of bidirectional type III bursts in solar flares.ASTROPHYSICS AND SPACE SCIENCE,318(1-2),87-92. |
| MLA | Ma, Y.,et al."Occurrence of bidirectional type III bursts in solar flares".ASTROPHYSICS AND SPACE SCIENCE 318.1-2(2008):87-92. |
入库方式： OAI收割
来源：国家天文台
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