DocumentCode :
3267001
Title :
Low noise temperature measurement methods in radio astronomy
Author :
Chen, Yong ; Sun, Zheng-Wen ; Wang Xiao-Mei ; Wang Si-xiu
Author_Institution :
Nat. Astron. Obs., Chinese Acad. of Sci., Urumqi, China
Volume :
5
fYear :
2010
fDate :
22-24 June 2010
Abstract :
Noise temperature of the receiver and low noise amplifier are become lower and lower with the fast development of electronic technique, it has become difficult to measure the noise temperature accurate and rapid. In this paper, various methods of noise temperature measurements in radio astronomy are described. The factors that influence the measurement precision also are discussed.
Keywords :
electric noise measurement; radioastronomy; radiofrequency interference; low noise amplifier; low noise temperature measurement; radio astronomy; Extraterrestrial measurements; HEMTs; Noise figure; Noise measurement; Power generation; Power measurement; Radio astronomy; Receivers; Signal to noise ratio; Temperature measurement; Noise temperature measurement; Y-factor; accuracy; hot and cold loads;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Education Technology and Computer (ICETC), 2010 2nd International Conference on
Conference_Location :
Shanghai
Print_ISBN :
978-1-4244-6367-1
Type :
conf
DOI :
10.1109/ICETC.2010.5529787
Filename :
5529787
Link To Document :
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