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Highly polarized type III microwave bursts on 15 April 1998
Wang M(汪敏)1; Duan, CC2; Xie RX(谢瑞祥)1; Yan, YH3; Wang, M (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
发表期刊SOLAR PHYSICS
2003-02
卷号212期号:2页码:401-406
DOI10.1023/A:1022939203483
产权排序第1完成单位
收录类别SCI
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.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0038-0938
URL查看原文
归档日期2003-08-13
WOS记录号WOS:000181818600011
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]BROAD-BAND SPECTROMETER ; ELECTRON-BEAMS ; SOLAR-BURSTS ; RADIO-BURSTS ; EMISSION ; FLARES ; TIME
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被引频次:2[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/5610
专题射电天文研究组
通讯作者Wang, M (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
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
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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,&Wang, M .(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.
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