1 October 1991 Receiver development with Nb/Al-oxide/Nb SIS mixers in the frequency ranges of 210-270 and 320-370 GHz
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Proceedings Volume 1576, 16th International Conference on Infrared and Millimeter Waves; 15761X (1991) https://doi.org/10.1117/12.2297782
Event: 16th International Conference on Infrared and Millimeter Waves, 1991, Lausanne, Switzerland
Abstract
For many years TRAM has used PbBi/in-oxide/Pb SIS mixers in the heterodyne receivers for radioastronomy at the telescope installations of Pico Veleta and Plateau de Bure. The frequency coverage of these receivers are (75-115)GHz, (130-180)GHz, and (210-270)GHz. The waveguide mixers, which use Nb/Al-oxide/Nb junctions are subjected to progressive updating. This paper concentrates on the work at (210-270)GHz and (320-370)GHz.
© (1991) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
M. C. Carter, M. C. Carter, } "Receiver development with Nb/Al-oxide/Nb SIS mixers in the frequency ranges of 210-270 and 320-370 GHz", Proc. SPIE 1576, 16th International Conference on Infrared and Millimeter Waves, 15761X (1 October 1991); doi: 10.1117/12.2297782; https://doi.org/10.1117/12.2297782
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