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Microwave patch structures on 12 June 1998
Wang M(汪敏)1,3; Fu, QJ2,3; Xie RX(谢瑞祥)1,3; Duan ZC(段长春)1,3; Wang, M (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Peoples R China.
发表期刊SOLAR PHYSICS
2001
卷号203期号:1页码:145-148
DOI10.1023/A:1012766308328
产权排序第1完成单位
收录类别SCI
摘要A microwave patch event observed with the 2.6-3.8 GHz spectrometer of Beijing Astronomical Observatory (BAO) on 12 June 1998 is described in detail in this paper. The patches show high flux densities, high polarization degree, extremely narrow bandwidth, and high spectral indexes. These observational characteristics may suggest that the favored emission mechanism is plasma or maser emission rather than gyrosynchrotron 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2002-03-13
WOS记录号WOS:000172172600011
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]RADIO-EMISSION ; SOLAR ; BURSTS ; DECIMETER
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被引频次:4[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/114a53/5600
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.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
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GB/T 7714
Wang M,Fu, QJ,Xie RX,et al. Microwave patch structures on 12 June 1998[J]. SOLAR PHYSICS,2001,203(1):145-148.
APA Wang M,Fu, QJ,Xie RX,Duan ZC,&Wang, M .(2001).Microwave patch structures on 12 June 1998.SOLAR PHYSICS,203(1),145-148.
MLA Wang M,et al."Microwave patch structures on 12 June 1998".SOLAR PHYSICS 203.1(2001):145-148.
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