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Low noise cryogenic receiver for spectroscopic applications in mm-wave radioastronomy at 230 GHz

Journal Article · · Microwave J.; (United States)
OSTI ID:6690846
A new cooled mm-wave receiver is presented. This receiver has been in operation since October 1985 with a 2.5 m Cassegrain telescope located at the Plateau de Bure in the French Alps. It is tunable from 210 to 240 GHz and has a DSB system noise temperature of 360 K and a 600 MHz instantaneous bandwidth. The receiver is composed of a local oscillator (klystron frequency tripler) and a Schottky diode mixer with a cooled FET amplifier. Quasi-optical techniques are used for signal injection. A computer-controlled microprocessor drives the whole system and performs calibration and frequency tuning of the receiver. The different parts of the receiver, frequency tripler, quasi-optical techniques, mixer, FET amplifier, and microprocessor, are described. 13 references.
Research Organization:
Meudon, Observatoire, France
OSTI ID:
6690846
Journal Information:
Microwave J.; (United States), Journal Name: Microwave J.; (United States) Vol. 29; ISSN MCWJA
Country of Publication:
United States
Language:
English

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