A broadband solar radio spectrometer and some new observational results
Xu, FY; Xu, ZC; Huang, GI; Yao, QJ; Meng, X; Wu, HA
刊名SOLAR PHYSICS
2003-09-01
卷号216期号:1-2页码:273-284
关键词FLARE YOHKOH BURSTS EMISSION DENSITY MODELS
ISSN号0038-0938
英文摘要A broadband solar radio spectrometer with a bandwidth of about 7 GHz has been developed in China for solar maximum 23. This work is a cooperative project of Beijing Astronomical Observatory (BAO), Purple Mountain Observatory (PMO), Yunnan Observatory (YNO), and Nanjing University. The spectrometer of PMO worked in the waveband of 4.5-7.5 GHz, that of BAO in 1-2 GHz,2.6-3.8 GHz, and 5.2-7.6 GHz, and that of YNO in 0.7-1.5 GHz. The spectrometer of PMO is a multichannel and frequency-agile one with a time resolution of 1-5 ms and a frequency resolution of 10 MHz. It started to operate in August 1999 and since then more than 300 spectral events have been observed, and some type III or type III-like structures have also been found. In this paper, some selected typical events, for example, the events on 25 August 1999 and 27 October 1999, are presented, and some new observed features are also described and discussed.
学科主题Astronomy & Astrophysics ; Mathematics
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]FLARE ; YOHKOH ; BURSTS ; EMISSION ; DENSITY ; MODELS
收录类别SCI
语种英语
WOS记录号WOS:000185962600018
公开日期2012-08-08
内容类型期刊论文
源URL[http://libir.pmo.ac.cn/handle/332002/4611]  
专题紫金山天文台_太阳活动的多波段观测研究团组
作者单位1.Chinese Acad Sci, Purple Mt Observ, Nanjing 21008, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
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GB/T 7714
Xu, FY,Xu, ZC,Huang, GI,et al. A broadband solar radio spectrometer and some new observational results[J]. SOLAR PHYSICS,2003,216(1-2):273-284.
APA Xu, FY,Xu, ZC,Huang, GI,Yao, QJ,Meng, X,&Wu, HA.(2003).A broadband solar radio spectrometer and some new observational results.SOLAR PHYSICS,216(1-2),273-284.
MLA Xu, FY,et al."A broadband solar radio spectrometer and some new observational results".SOLAR PHYSICS 216.1-2(2003):273-284.
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