PMO OpenIR  > 太阳活动的多波段观测研究团组
Slowly Drifting Radio Structures in Solar Flares
Ning Zongjun ; Wu Hongao ; Xu Fuying ; Meng Xuan
2012
Source PublicationAstronomical Research & Technology
ISSN1672-7673
Volume9Issue:4Pages:363-365
AbstractWe present the data of high-frequency drift radio structures observed by the spectrometer of the Purple Mountain Observatory(PMO) over the frequency range of 4.5-7.5GHz in the solar flare of March 18,2003.Such structures have been observed to have fine features consisting of short pulses,but drift with time as a whole.The drifting structures take place before the soft X-ray maximum,almost at the maximum of hard X-ray flux of 25-50keV.For the first time,drifts toward higher frequencies are detected in this kind of radio structures near 6GHz.
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8137
Collection太阳活动的多波段观测研究团组
Recommended Citation
GB/T 7714
Ning Zongjun,Wu Hongao,Xu Fuying,et al. Slowly Drifting Radio Structures in Solar Flares[J]. Astronomical Research & Technology,2012,9(4):363-365.
APA Ning Zongjun,Wu Hongao,Xu Fuying,&Meng Xuan.(2012).Slowly Drifting Radio Structures in Solar Flares.Astronomical Research & Technology,9(4),363-365.
MLA Ning Zongjun,et al."Slowly Drifting Radio Structures in Solar Flares".Astronomical Research & Technology 9.4(2012):363-365.
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