中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Microwave Type U and RS Bursts in the X2.2 Solar Flare on 15 February 2011

文献类型:期刊论文

作者Xue Yu1; Wang Shujuan1; Yan Yihua1; Huang Chong1; Yu Sijie3; Wang Rui2
刊名Chinese Journal of Space Science
出版日期2015
卷号35期号:2页码:135
关键词Solar flare Solar radio microwave burst
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/114a11/60200]  
专题中国科学院国家天文台
作者单位1.中国科学院国家天文台
2.中国科学院
3.Max-Planck Institute for Solar System, Justus-uon-Liebig-Weg-3
推荐引用方式
GB/T 7714
Xue Yu,Wang Shujuan,Yan Yihua,et al. Microwave Type U and RS Bursts in the X2.2 Solar Flare on 15 February 2011[J]. Chinese Journal of Space Science,2015,35(2):135.
APA Xue Yu,Wang Shujuan,Yan Yihua,Huang Chong,Yu Sijie,&Wang Rui.(2015).Microwave Type U and RS Bursts in the X2.2 Solar Flare on 15 February 2011.Chinese Journal of Space Science,35(2),135.
MLA Xue Yu,et al."Microwave Type U and RS Bursts in the X2.2 Solar Flare on 15 February 2011".Chinese Journal of Space Science 35.2(2015):135.

入库方式: OAI收割

来源:国家天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。