30 November 2017 Low-noise quasioptical 2-mm mixer receiver
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Proceedings Volume 2250, International Conference on Millimeter and Submillimeter Waves and Applications 1994; 22507R (2017) https://doi.org/10.1117/12.2303296
Event: Millimeter and Submillimeter Waves and Applications: International Conference, 1994, San Diego, CA, United States
Abstract
Quasioptical radioastronomical 2-mm mixer receiver for room temperature operation are described. Receiver incorporates polarization-rotating dual-beam quasioptical interferometer, waveguide Schottky mixer, carcinotron LO, GaAs IF amplifier. The best receiver noise temperature is 600 K (DSB) at 136 GHz.
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
I. I. Eru, I. I. Eru, } "Low-noise quasioptical 2-mm mixer receiver", Proc. SPIE 2250, International Conference on Millimeter and Submillimeter Waves and Applications 1994, 22507R (30 November 2017); doi: 10.1117/12.2303296; https://doi.org/10.1117/12.2303296
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