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A group of solar microwave type-III bursts on 1998 April 15
Duan, CC; Wang, M; Xie, RX; Yan, YH
2002-04-01
Source PublicationCHINESE ASTRONOMY AND ASTROPHYSICS
Volume26Issue:2Pages:189-197
AbstractWe describe in detail a group of microwave type-III bursts observed on 1998 April 15 by the 2.6-3.8 GHz solar radio spectrometer of Beijing Astronomical Observatory. The bursts are characterised by broad bandwidths (> 100 MHz), short durations (< 100 ms), very high degrees of polarization (&SIM; 100%), positive rates of frequency drifts (> 1 GHz/s) and fast pulsations (with periods of about 100 ms). Their time profiles are also analyzed. According to these characteristics, we suggest that they originate from plasma fundamental wave emission.
KeywordSun Microwave Type-iii Burst Plasma Radiation
Indexed BySCI
Language英语
WOS IDWOS:000176345300008
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8550
Collection太阳物理研究部
Affiliation1.Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Duan, CC,Wang, M,Xie, RX,et al. A group of solar microwave type-III bursts on 1998 April 15[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2002,26(2):189-197.
APA Duan, CC,Wang, M,Xie, RX,&Yan, YH.(2002).A group of solar microwave type-III bursts on 1998 April 15.CHINESE ASTRONOMY AND ASTROPHYSICS,26(2),189-197.
MLA Duan, CC,et al."A group of solar microwave type-III bursts on 1998 April 15".CHINESE ASTRONOMY AND ASTROPHYSICS 26.2(2002):189-197.
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