microwavetypeuandrsburstsinthex22solarflareon15february2011
文献类型：期刊论文
| 作者 | Xue Yu3; Wang Shujuan3 ; Yan Yihua3; Huang Chong3; Yu Sijie2; Wang Rui1
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| 刊名 | 空间科学学报
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| 出版日期 | 2015 |
| 卷号 | 35期号:2页码:135 |
| ISSN号 | 0254-6124 |
| 英文摘要 | Two groups of microwave type U and Reverse-Slope (RS) bursts after the Soft X-Ray (SXR) maximum were observed with the 2.6~3.8 GHz spectrometer of Chinese Solar Broadband Radio Spectrometers (SBRS/Huairou) on 15 February 2011, when an X2.2 solar flare occurred in the Active Region (AR) NOAA11158. A Shear-driven Quadrupolar Reconnection (SQR) model was utilized to analyze these bursts and the two loops involved were found to be basically in the same spatial scale and have a height difference of about 1300 km. These bursts were interpreted to be a result of a new reconnection process between the two similar-scaled loops. |
| 语种 | 英语 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/46330]  |
| 专题 | 中国科学院国家天文台 |
| 作者单位 | 1.中国科学院 2.Max-Planck Institute for Solar System, Justus-uon-Liebig-Weg-3 3.中国科学院国家天文台 |
| 推荐引用方式 GB/T 7714 | Xue Yu,Wang Shujuan,Yan Yihua,et al. microwavetypeuandrsburstsinthex22solarflareon15february2011[J]. 空间科学学报,2015,35(2):135. |
| APA | Xue Yu,Wang Shujuan,Yan Yihua,Huang Chong,Yu Sijie,&Wang Rui.(2015).microwavetypeuandrsburstsinthex22solarflareon15february2011.空间科学学报,35(2),135. |
| MLA | Xue Yu,et al."microwavetypeuandrsburstsinthex22solarflareon15february2011".空间科学学报 35.2(2015):135. |
入库方式： OAI收割
来源：国家天文台
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