中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Highly polarized type III microwave bursts on 15 April 1998

文献类型:期刊论文

作者Wang M(汪敏)1; Duan, CC2; Xie RX(谢瑞祥)1; Yan, YH3
刊名SOLAR PHYSICS
出版日期2003-02
卷号212期号:2页码:401-406
ISSN号0038-0938
产权排序第一完成单位
通讯作者Wang, M (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
英文摘要A group of type III bursts observed with the 2.6-3.8 GHz spectrometer of National Astronomical Observatory of China on 15 April 1998 is analyzed. They have the characteristics of broad bandwidth (>100 MHz), very short durations (<100 ms), high polarization degree (&AP;100%), high frequency drift rates (>1 GHz s(-1)), and fast pulsations (with a period of about 100-200 ms). Their time profiles are also analysed. According to these characteristics, we suggest that these microwave type III bursts may be due to the fundamental plasma emission.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]BROAD-BAND SPECTROMETER ; ELECTRON-BEAMS ; SOLAR-BURSTS ; RADIO-BURSTS ; EMISSION ; FLARES ; TIME
收录类别SCI
原文出处http://link.springer.com/article/10.1023%2FA%3A1022939203483
语种英语
WOS记录号WOS:000181818600011
源URL[http://ir.ynao.ac.cn/handle/114a53/5610]  
专题云南天文台_射电天文研究组
作者单位1.National Astronomical Observatory/Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, China
2.Yunnan Meteorological Institute of Science, Kunming, 650034, China
3.National Astronomical Observatory, Chinese Academy of Sciences, Beijing, 100012, China
推荐引用方式
GB/T 7714
Wang M,Duan, CC,Xie RX,et al. Highly polarized type III microwave bursts on 15 April 1998[J]. SOLAR PHYSICS,2003,212(2):401-406.
APA Wang M,Duan, CC,Xie RX,&Yan, YH.(2003).Highly polarized type III microwave bursts on 15 April 1998.SOLAR PHYSICS,212(2),401-406.
MLA Wang M,et al."Highly polarized type III microwave bursts on 15 April 1998".SOLAR PHYSICS 212.2(2003):401-406.

入库方式: OAI收割

来源:云南天文台

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