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Construction of a 345-gigahertz receiver based on superconducting tunnel junctions. Final report, 1 October 1985-31 December 1989

Technical Report ·
OSTI ID:7120769
This report describes the construction of a 345 Gigahertz receiver system based on superconducting tunnel junctions. The junctions used are Niobium edge junctions, which are mounted in a waveguide mixer mount. Highest sensitivity occurs at 312 GHz with a measured receiver noise temperature of 275 K double sideband. Theoretical calculations and experimental results both indicate the likelihood of good low noise operation out to 1000 GHz using techniques of the sort described here. (rrh)
Research Organization:
California Univ., Berkeley, CA (USA). Space Sciences Lab.
OSTI ID:
7120769
Report Number(s):
AD-A-218781/3/XAB
Country of Publication:
United States
Language:
English