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Characteristics of the radio emission of solar white-light flares: Moving type-IV bursts and short-period pulsations associated with post-flare loops
Xie RX(谢瑞祥)1,2,3; Wang M(汪敏)1,2,3; Xie, RX
Source PublicationCHINESE ASTRONOMY AND ASTROPHYSICS
2000-04
Volume24Issue:2Pages:241-249
DOI10.1016/S0275-1062(00)00048-5
Contribution Rank第1完成单位
Indexed BySCI
KeywordWhite-night Flare Radio Burst Post-flare Loop Radio Pulsation
AbstractWe analyse in depth the complex solar event of 1991-06-06 comprising a broad-band moving type-IV radio burst, a white light flare occurring during the impulsive phase of an Ho flare, a post-flare loop and its multiple period (1-4s) radio pulsation in an investigation of their relationship and status of association.
Language英语
Subject AreaAstronomy & Astrophysics
SubtypeArticle
ISSN0275-1062
URL查看原文
WOS IDWOS:000087315900012
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordMAGNETIC-FIELD ; REGION
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Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/5594
Collection射电天文研究组
Corresponding AuthorXie, RX
Affiliation1.Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011 ROC
2.Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012 ROC
3.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 ROC
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Xie RX,Wang M,Xie, RX. Characteristics of the radio emission of solar white-light flares: Moving type-IV bursts and short-period pulsations associated with post-flare loops[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2000,24(2):241-249.
APA Xie RX,Wang M,&Xie, RX.(2000).Characteristics of the radio emission of solar white-light flares: Moving type-IV bursts and short-period pulsations associated with post-flare loops.CHINESE ASTRONOMY AND ASTROPHYSICS,24(2),241-249.
MLA Xie RX,et al."Characteristics of the radio emission of solar white-light flares: Moving type-IV bursts and short-period pulsations associated with post-flare loops".CHINESE ASTRONOMY AND ASTROPHYSICS 24.2(2000):241-249.
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