A full-band waveguide SIS receiver with integrated tuning for 75-110 GHz
Autor: | P. F. Goldsmith, N. R. Erickson, N. G. Ugras, A. H. Worsham, Dag Winkler, Daniel E. Prober |
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Rok vydání: | 1991 |
Předmět: |
Noise temperature
Materials science business.industry Frequency band Local oscillator Niobium chemistry.chemical_element Inductor Diffusion capacitance Chebyshev filter Electronic Optical and Magnetic Materials law.invention chemistry law Optoelectronics Electrical and Electronic Engineering business Transformer |
Zdroj: | IEEE Transactions on Magnetics. 27:2634-2637 |
ISSN: | 1941-0069 0018-9464 |
DOI: | 10.1109/20.133752 |
Popis: | The performance of a broadband SIS (superconductor-insulator-superconductor) receiver with no mechanical tuning elements was modeled and tested. The mixer mount had a broadband-waveguide-to-microstripline transition consisting of a four-step Chebyshev single-ridge transformer. The last step of the ridge connected the waveguide to a microstripline circuit. The on-chip circuit consisted of a microstripline that transmitted the RF and the local oscillator signals to the SIS mixer. Both the SIS element and the inductor had RF grounds provided by 90 degrees radial stubs. The inductor tuned out the junction capacitance to allow operation over the full frequency band. The SIS element can be a single junction or series array using Nb-AlO/sub x/-Nb trilayer tunnel junctions with areas as small as 0.5 mu m/sup 2/ and V/sub m/(2 mV)=39 mV. Preliminary results indicated a DSB receiver noise temperature of 65-80 K across the band measured at 4.4 K with an internal cryogenic RF hot/cold source and with T/sub if/=21 K. With another device, a mixer noise temperature of 35 K at 100 GHz was achieved, increasing to 45 K at 79.5 and 110 GHz. Coupled mixer gain of up to +3 dB and negative dynamic resistance on the first photon step were observed. The lowest noise temperature was obtained for an untuned single-junction mixer at 80 GHz: T/sub R/=41 K and T/sub M/=20 K were measured. |
Databáze: | OpenAIRE |
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