中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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
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

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。