NAOC Open IR
microwavetypeuandrsburstsinthex22solarflareon15february2011
Xue Yu1; Wang Shujuan1; Yan Yihua1; Huang Chong1; Yu Sijie2; Wang Rui3
2015
Source Publication空间科学学报
ISSN0254-6124
Volume35Issue:2Pages:135
AbstractTwo 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.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/46331
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.Max-Planck Institute for Solar System, Justus-uon-Liebig-Weg-3
3.中国科学院
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
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.
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