中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Solar Partial N-burst

文献类型:期刊论文

作者Ning Zongjun1; Liu Yuying1; Fu Qijun1; Xu Fuying2
刊名Chinese Journal of Astronomy and Astrophysics
出版日期2003
卷号3期号:4页码:381
ISSN号1009-9271
英文摘要We present a new sub-class of type III solar radio burst at the highfrequencies around 6.0 GHz. In addition to a descending and an ascending branchon the dynamic spectrum, it has an inverted morphology different from the simpletype U-burst. We call it "partial N-burst" because it is interpreted as the knownN-burst minus its first branch. The partial N-burst presented here was detectedamong a reverse slope type III (RS-III) burst group prior to the type V solar radiocontinuum and was simultaneously recorded by two spectrometers at the NationalAstronomical Observatories, Chinese Academy of Sciences (NAOC, 5.20-7.60 GHz)and at Purple Mountain Observatory (PMO, 4.50-7.50 GHz) on 1999 August 25.After the N-burst and M-burst, the partial N-burst is a third piece of evidence for amagnetic mirror effect in solar radio observation, when the same electron is reflectedat a pinched foot of a flare loop.
语种英语
源URL[http://ir.bao.ac.cn/handle/114a11/38123]  
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.中国科学院紫金山天文台
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GB/T 7714
Ning Zongjun,Liu Yuying,Fu Qijun,et al. Solar Partial N-burst[J]. Chinese Journal of Astronomy and Astrophysics,2003,3(4):381.
APA Ning Zongjun,Liu Yuying,Fu Qijun,&Xu Fuying.(2003).Solar Partial N-burst.Chinese Journal of Astronomy and Astrophysics,3(4),381.
MLA Ning Zongjun,et al."Solar Partial N-burst".Chinese Journal of Astronomy and Astrophysics 3.4(2003):381.

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来源:国家天文台

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