Microwave Type U and RS Bursts in the X2.2 Solar Flare on 15 February 2011

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	Microwave Type U and RS Bursts in the X2.2 Solar Flare on 15 February 2011
	Xue Yu 1; Wang Shujuan1 ; Yan Yihua1 ; Huang Chong 1; Yu Sijie 2; Wang Rui 3
	2015
Source Publication	Chinese Journal of Space Science
ISSN	0254-6124
Volume	35 Issue:2 Pages:135
Abstract	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.
Keyword	Solar flare Solar radio microwave burst
Language	英语
Document Type	期刊论文
Identifier	http://ir.bao.ac.cn/handle/114a11/60201
Collection	中国科学院国家天文台
Affiliation	1.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 Affilication	National Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation 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.

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