30 August 1993 A sub-millimetre wave SIS receiver
Author Affiliations +
Proceedings Volume 2104, 18th International Conference on Infrared and Millimeter Waves; 21041J (1993) https://doi.org/10.1117/12.2298487
Event: 18th International Conference on Infrared and Millimeter Waves, 1993, Colchester, United Kingdom
A superconducting (SIS) tunnel junction heterodyne receiver has been constructed and tested over the frequency range450 to 540 GHz. The receiver uses a reduced height waveguide mount and a Pb alloy tunnel junction as the detectingelement. Performance measurements made with the receiver installed on the James Clerk Maxwell Telescope, Hawaii,show a noise temperature (DSB) of 165 K at 460 GHz and 220 K at 490 GHz, measured in a 1 GHz instantaneous IFbandwidth centred at 4 GHz. The receiver demonstrates that Pb alloy junctions are sufficiently stable and reliable toallow use at a remote observing site at sub-millimetre wavelengths.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
B. N. Ellison, "A sub-millimetre wave SIS receiver", Proc. SPIE 2104, 18th International Conference on Infrared and Millimeter Waves, 21041J (30 August 1993); doi: 10.1117/12.2298487; https://doi.org/10.1117/12.2298487


Sis-mixers around the gap frequency
Proceedings of SPIE (January 01 1994)
A sub millimetre wave SIS receiver for the James Clerk...
Proceedings of SPIE (November 30 2017)
SIS-mixer development at SRON
Proceedings of SPIE (August 30 1993)
Noise properties of a mixer with SIS NbN quasi particle...
Proceedings of SPIE (October 13 1995)
A 275 to 370 GHz SIS mixer for the...
Proceedings of SPIE (October 08 2004)

Back to Top