Paper
1 October 1991 Receiver development with Nb/Al-oxide/Nb SIS mixers in the frequency ranges of 210-270 and 320-370 GHz
Author Affiliations +
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 "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); https://doi.org/10.1117/12.2297782
Lens.org Logo
CITATIONS
Cited by 2 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Receivers

Waveguides

Magnetism

Temperature metrology

Electrodes

Lead

Linear filtering

RELATED CONTENT

A sub millimetre wave SIS receiver for the James Clerk...
Proceedings of SPIE (November 30 2017)
A sub-millimetre wave SIS receiver
Proceedings of SPIE (August 30 1993)
A 385 to 500 GHz SIS mixer the for APEX...
Proceedings of SPIE (July 06 2006)
High sensitivity 810 GHz SIS receivers at AST/RO
Proceedings of SPIE (October 08 2004)
A 275 to 370 GHz SIS mixer for the...
Proceedings of SPIE (October 08 2004)

Back to Top