Solar Partial N-burst
文献类型:期刊论文
作者 | Ning Zongjun1; Liu Yuying1![]() ![]() |
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 |
推荐引用方式 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. |
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。