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Observational characteristics of weak polarized microwave spikes
Wang M(汪敏)1,2,4; Fu, QJ1,4; Xie RX(谢瑞祥)1,2,4; Huang, GL3,4; Wang, M
发表期刊SOLAR PHYSICS
1999-10
卷号189期号:2页码:331-344
DOI10.1023/A:1005213701438
产权排序第2完成单位
收录类别SCI
摘要Eleven microwave spike events observed with the 2.6-3.8 GHz spectrometer of Beijing Astronomical Observatory (BAO) are analysed. The polarization degrees of spikes are variable, some spikes have frequency drift with the drift rate of several GHz s(-1). In particular, the time delay (8 ms) between the two polarization modes of spike is detected, which is different from previous results. According to the leading spot rule, we conclude that the o-modes arrive first. Moreover, the reversal of polarization sense versus frequency is also found. A change of the emission mode may be the cause of the polarization reversal.
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1999-12-31
WOS记录号WOS:000085034200008
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]RADIO SPIKES ; SOLAR CORONA ; BURSTS ; FLARE ; SCATTERING ; EMISSION ; WAVES
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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/114a53/5590
专题射电天文研究组
通讯作者Wang, M
作者单位1.1Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012, China
2.2Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China
3.3Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China
4.4National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 , China
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Wang M,Fu, QJ,Xie RX,et al. Observational characteristics of weak polarized microwave spikes[J]. SOLAR PHYSICS,1999,189(2):331-344.
APA Wang M,Fu, QJ,Xie RX,Huang, GL,&Wang, M.(1999).Observational characteristics of weak polarized microwave spikes.SOLAR PHYSICS,189(2),331-344.
MLA Wang M,et al."Observational characteristics of weak polarized microwave spikes".SOLAR PHYSICS 189.2(1999):331-344.
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