DocumentCode :
2068197
Title :
New Millimetrewave Receivers at NRAO
Author :
Lamb, James W. ; Payne, John M. ; Bailey, Nancyjane
Author_Institution :
National Radio Astronomy Observatory, 949 N. Cherry Ave., Campus Bldg. 65, Tucson, Arizona 85721-0655, USA
Volume :
2
fYear :
1992
fDate :
5-9 Sept. 1992
Firstpage :
975
Lastpage :
980
Abstract :
A new generation of low-noise, dual-polarisation receivers covering the atmospheric windows between 65 GHz and 300 GHz is nearing completion. These receivers use niobium junction SIS mixers which have proven to be very sensitive and reliable. A modular approach has been used and each receiver channel is constructed as an insert which is mounted in a stainless-steel dewar cooled by a closed-cycle 4K refrigerator. Several frequency bands may be accommodated in a single package. Currently, a 65-116 GHz receiver with noise temperatures typically <1OOK SSB, a 130-170 GHz with noise temperatures typically <200K, and a 200-270 GHz receiver with noise temperatures typically <200K SSB are operational. A 260-300 GHz insert is under construction.
Keywords :
Amplitude modulation; Frequency; Lenses; Niobium; Optical receivers; Packaging; Radio astronomy; Refrigeration; Telescopes; Temperature;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Microwave Conference, 1992. 22nd European
Conference_Location :
Helsinki, Finland
Type :
conf
DOI :
10.1109/EUMA.1992.335831
Filename :
4135576
Link To Document :
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