New solar broadband radio spectrometer (SBRS) in China

doi:10.1023/B:SOLA.0000036876.14446.dd

YNAO OpenIR > 射电天文研究组

	New solar broadband radio spectrometer (SBRS) in China
	Fu, QJ 1; Ji, HR 1; Qin, ZH 2; Xu, ZC 3; Xia ZG(夏志国)4 ; Wu, HG 3; Liu, YY 1; Yan, YH 1; Huang, GL 3; Chen, ZJ 1; Jin ZY(金振宇)4 ; Yao, QJ 3; Cheng, CL 1; Xu, FY3 ; Wang M(汪敏)4 ; Pei, LB 3; Chen, SH 3; Yang, G 2; Tan, CM 1; Shi SB(施硕彪)4 ; Fu, QJ (reprint author), Chinese Acad Sci, Natl Astron Observ NAOC, Beijing 100012, Peoples R China.
发表期刊	SOLAR PHYSICS
	2004-07
卷号	222 期号:1 页码:167-175
DOI	10.1023/B:SOLA.0000036876.14446.dd
产权排序	第3完成单位
收录类别	SCI
摘要	A new radio spectrometer, Solar Broadband Radio Spectrometer (SBRS) with characteristics of high time resolution, high-frequency resolution, high sensitivity, and wide frequency coverage in the microwave region is described. Its function is to monitor solar radio bursts in the frequency range of 0.7-7.6 GHz with time resolution of 1-10 ms. SBRS consists of five 'component spectrometers' which work in five different wave bands (0.7-1.5 GHz, 1.0-2.0 GHz, 2.6-3.8 GHz, 4.5-7.5 GHz, and 5.2-7.6 GHz, respectively). A combination of multi-channel and scanning techniques is adopted. The component spectrometers are attached to different antennas which are separately located at Beijing, Kunming, and Nanjing. Close attention was paid to solve the problems of sensitivity, dynamic range, interference-resistance, data acquisition, and handling a large amount of data. The SBRS was put into operation in the 23th solar maximum activity period, and has proved itself to be a valuable instrument for the study of solar bursts in microwaves.
语种	英语
学科领域	Astronomy & Astrophysics
文章类型	Article
ISSN	0038-0938
URL	查看原文
WOS记录号	WOS:000223093800011
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	FINE-STRUCTURES ; MICROWAVE-BURSTS ; ONDREJOV RADIOSPECTROGRAPH ; FREQUENCY-RANGE ; APRIL 15 ; 3 GHZ ; SPIKES ; CATALOG ; FLARES ; REGION
引用统计	被引频次：93[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/114a53/5613
专题	射电天文研究组
通讯作者	Fu, QJ (reprint author), Chinese Acad Sci, Natl Astron Observ NAOC, Beijing 100012, Peoples R China.
作者单位	1.National Astronomical Observatories (NAOC), Chinese Academy of Sciences, Beijing, 100012, China 2.Department of Astronomy, Nanjing University (NJU), Nanjing, 210093, China 3.Purple Mountain Observatory (PMO), Chinese Academy of Sciences, Nanjing, 210008, China 4.Yunnan Astronomical Observatory (YAO), National Astronomical Observatories, Chinese Academy of Sciences, Yunnan, 650011, China
推荐引用方式 GB/T 7714	Fu, QJ,Ji, HR,Qin, ZH,et al. New solar broadband radio spectrometer (SBRS) in China[J]. SOLAR PHYSICS,2004,222(1):167-175.
APA	Fu, QJ.,Ji, HR.,Qin, ZH.,Xu, ZC.,Xia ZG.,...&Fu, QJ .(2004).New solar broadband radio spectrometer (SBRS) in China.SOLAR PHYSICS,222(1),167-175.
MLA	Fu, QJ,et al."New solar broadband radio spectrometer (SBRS) in China".SOLAR PHYSICS 222.1(2004):167-175.

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文件名称/大小	文献类型	版本类型	开放类型	使用许可
A New Solar Broadban（269KB）	期刊论文	作者接受稿	开放获取	CC BY-NC-SA	浏览请求全文