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Low-noise receivers: S-band parametric up converter developmentThe combination of a cryogenically-cooled parametric upconverter and a higher frequency maser post amplifier was proposed as a method of achieving maser-like receiver noise temperatures over much larger instantaneous bandwidths and tuning ranges than are presently obtainable with masers in the range of 1 to 18 GHz. An experimental 2.0- to 2.5-GHz parametric upconverter/maser system was developed to explore these possibilities. Initial tests of this system resulted in an effective input noise temperature of 3.1 K at 2295 MHz and 3.2 K at 2388 MHz. The parametric upconverter logged over 1500 hours at 4.5 K and underwent 5 thermal cycles (300 K to 4.5 K to 300 K) without degradation.
Document ID
19790007837
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Petty, S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Neff, D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Norris, D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 10, 2013
Publication Date
December 15, 1978
Publication Information
Publication: The Deep Space Network
Subject Category
Communications And Radar
Accession Number
79N16008
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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