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Highly polarized type III microwave bursts on 15 April 1998
Wang, M; Duan, CC; Xie, RX; Yan, AH
2003-02-01
Source PublicationSOLAR PHYSICS
Volume212Issue:2Pages:401-406
AbstractA 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.
Indexed BySCI
Language英语
WOS IDWOS:000181818600011
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Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8434
Collection太阳物理研究部
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China
2.Yunnan Meteorol Inst Sci, Kunming 650034, Peoples R China
3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
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, AH.(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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