Highly polarized type III microwave bursts on 15 April 1998
文献类型:期刊论文
作者 | Wang, M; Duan, CC; Xie, RX; Yan, AH |
刊名 | SOLAR PHYSICS
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出版日期 | 2003-02-01 |
卷号 | 212期号:2页码:401-406 |
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. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000181818600011 |
源URL | [http://ir.bao.ac.cn/handle/114a11/8434] ![]() |
专题 | 国家天文台_太阳物理研究部 |
作者单位 | 1.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 |
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, 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. |
入库方式: OAI收割
来源:国家天文台
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