Observations of microwave type-U bursts

doi:10.1023/A:1010301632136

YNAO OpenIR > 射电天文研究组

	Observations of microwave type-U bursts
	Wang M(汪敏)1,4 ; Fu, QJ 2,4; Xie RX(谢瑞祥)1,4 ; Huang, GL 3,4; Duan ZC(段长春)1,4 ; Wang, M (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Peoples R China.
发表期刊	SOLAR PHYSICS
	2001-03
卷号	199 期号:1 页码:157-164
DOI	10.1023/A:1010301632136
产权排序	第1完成单位
收录类别	SCI
摘要	Two microwave type-U bursts observed with the 2.6-3.8 GHz spectrometer of Beijing Astronomical Observatory (BAO) are described and analysed in this paper. The microwave type-U bursts have very short durations (about 200 ms), narrow bandwidth. high-frequency drift rates of the ascending and descending branches, and a high degree of circular polarization (80%). The sense of polarization remains the same from the ascending to the descending branch.
语种	英语
学科领域	Astronomy & Astrophysics
文章类型	Article
ISSN	0038-0938
URL	查看原文
归档日期	2001-09-12
WOS记录号	WOS:000168585100013
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	RADIO-BURSTS ; SOLAR
引用统计	被引频次：9[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/114a53/5599
专题	射电天文研究组
通讯作者	Wang, M (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Peoples R China.
作者单位	1.Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming, 650011, China 2.Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing, 100012, China 3.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210008, China 4.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 , China
第一作者单位	中国科学院云南天文台
推荐引用方式 GB/T 7714	Wang M,Fu, QJ,Xie RX,et al. Observations of microwave type-U bursts[J]. SOLAR PHYSICS,2001,199(1):157-164.
APA	Wang M,Fu, QJ,Xie RX,Huang, GL,Duan ZC,&Wang, M .(2001).Observations of microwave type-U bursts.SOLAR PHYSICS,199(1),157-164.
MLA	Wang M,et al."Observations of microwave type-U bursts".SOLAR PHYSICS 199.1(2001):157-164.

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