Highly polarized type III microwave bursts on 15 April 1998

	Highly polarized type III microwave bursts on 15 April 1998
	Wang M(汪敏)1; Duan, CC 2; Xie RX(谢瑞祥)1; Yan, YH 3
刊名	SOLAR PHYSICS
	2003-02
卷号	212 期号:2 页码:401-406
ISSN号	0038-0938
通讯作者	Wang, M (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
产权排序	第一完成单位
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.
学科主题	Astronomy & Astrophysics
WOS标题词	Science & Technology ; Physical Sciences
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
内容类型	期刊论文
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.