YNAO OpenIR  > 射电天文研究组
Alternative TitleDesign of An Analog Receiver for Solar Radio Observation in the Frequency Range of 30MHz to 65MHz
郭少杰; 汪敏; 董亮; 施硕彪
Source Publication天文研究与技术(Astronomical Research & Technology)
Contribution Rank第1完成单位
Indexed ByCSCD
Keyword动态范围 低噪声系数 最小可测流量密度

10 m波段的太阳射电观测,对监测日冕物质抛射(Coronal Mass Ejection,CME)有着重要的意义。介绍了一种安装在太阳射电天线阵的模拟接收机,工作频率范围是30~65 MHz,用于监测太阳10 m波的爆发活动。接收机采用直接采样的结构,由巴伦、滤波器和放大器组成。研制完成的接收机,增益达到60 d B,动态范围约33 d B,输入三阶互调点IIP3=-24 d Bm,噪声系数N=4.3 d B,满足观测要求。最后,计算了太阳射电天线阵的最小可测流量密度。

Other Abstract

Solar radio radiations mainly come from the corona of the sun,and radio waves in different bands reflect activities in different layers of the corona. Observational studies about solar radio radiations are among the most important approaches to derive physical-parameter values of the corona ( e. g.,temperature, density,and magnetic-field strength) . Decimeter waves come from a corona layer of heights approximately 1 to 2 times of the solar radius above the solar surface,which makes solar radio observations in decimeter waves particularly important in the coronal physics. For example,such studies can be used to monitor propagations of CME ( Coronal Mass Ejection) and shock waves in high layers of the corona,and to forecast space weather. Currently,there is a lack of solar radio observations in decimeter waves in China. It is urgent to build Chinese decimeter-wave solar radio telescopes and associated key equipments. A solar radio antenna array working in low-frequency bands has been built in the YNAO ( Yunnan Observatories) . The array consists of four antennas. It will work with the YNAO 10m solar radio telescope ( working in the frequency range of 625MHz to 1500MHz) and 11m solar radio telescope ( working in the frequency range of 70MHz to 700MHz) ,achieving a complete wavelength coverage of coronal radio observation. In this paper we introduce our design of an analog receiver to be installed in the solar radio antenna array of the YNAO. The receiver is to monitor solar radio bursts in decimeter wavelengths corresponding to the frequency range of 30MHz to 65MHz. The analog receiver consists of Baluns,filters,and amplifiers for direct sampling. The performance parameters of the analog receiver meet the requirements for observations: The gain reaches 60dB,the dynamic range is about 33dB, the input third-order intercept point is about - 24dBm,and the noise figure is about 4. 3dB. We finally calculate the sensitivity limits of the solar radio antenna array with the analog receiver installed.

Funding Project国家自然科学基金[U1431113] ; 国家自然科学基金[11173010]
Funding Organization国家自然科学基金[U1431113, 11173010]
Subject Area天文学 ; 射电天文学 ; 射电天文方法
MOST Discipline Catalogue理学 ; 理学::天文学
Archive Date2016-01-06
Citation statistics
Document Type期刊论文
Affiliation中国科学院云南天文台,云南,昆明 650011
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
郭少杰,汪敏,董亮,等. 太阳射电30~65MHz波段模拟接收机的研制[J]. 天文研究与技术(Astronomical Research & Technology),2015,12(2):142-148.
APA 郭少杰,汪敏,董亮,&施硕彪.(2015).太阳射电30~65MHz波段模拟接收机的研制.天文研究与技术(Astronomical Research & Technology),12(2),142-148.
MLA 郭少杰,et al."太阳射电30~65MHz波段模拟接收机的研制".天文研究与技术(Astronomical Research & Technology) 12.2(2015):142-148.
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