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Radio Behavior of Solar Post-Flare Loops
Wang M(汪敏)1; Xie RX(谢瑞祥)1; Chen HD(陈华东)1; Yan, YH2
Source PublicationProceedings of the 233rd Symposium of the International Astronomical Union (IAU)- Solar Activity and its Magnetic Origin
2006
Volume233
Pages69-70
DOI10.1017/S1743921306001463
Author of SourceVolker Bothmer; Ahmed Abdel Hady
Contribution Rank第1完成单位
Indexed By其他
Conference Namethe 233rd Symposium of the International Astronomical Union (IAU)
Conference Date2006-03-31
Conference PlaceCairo, Egypt
KeywordSun: Radio Radiation
Abstract

The spectral and source characteristics of a complex radio burst observed with the spectrometers of China and the Nobeyama Radio Heliograph are analyzed. This burst presents two separate burst peaks occurred in different frequency range (broad-band microwave and narrow-band decimeter wavelengths). We stress that the late phase radio bursts in decimeter wavelength corresponding to the post-flare loops may be the radio homologous flare.

Funding OrganizationN/A
Language英语
Subject Area天文学 ; 射电天文学 ; 太阳与太阳系
MOST Discipline Catalogue理学 ; 理学::天文学
PublisherCambridge University Press
Publication PlaceCambridge
URL查看原文
Archive Date2007-09-12
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Document Type会议论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6554
Collection太阳物理研究组
Affiliation1.Yunnan Observatory, National Astronomical Observatories, CAS, Kunming 650011, China
2.National Astronomical Observatories, CAS, Beijing 100012, China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Wang M,Xie RX,Chen HD,et al. Radio Behavior of Solar Post-Flare Loops[C]//Volker Bothmer; Ahmed Abdel Hady. Cambridge:Cambridge University Press,2006:69-70.
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