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Superconductor Science and Technology

Ultra-low-noise 100 GHz receiver based on parallel biased SIS arrays

S. V. Shitov, V. P. Koshelets, Sergey Kovtonyuk, An. B. Ermakov, Nick D. Whyborn, C -O Lindstrom

Published Sep 1, 1991• 15 citations
Publisher

Abstract

The possibility of overcoming the main drawbacks of the traditional series arrays by using a parallel connection of SIS junctions for DC and IF current has been experimentally demonstrated in full height 70-116 GHz waveguide mixers. This new array concept has been successfully developed to: (i) avoid the influence of junction non-uniformity in the array; (ii) provide optimal matching at both RF input and IF output even in the case of high gain, and (iii) tune out junction capacitance without any DC blocks. The experimentally tested arrays contain 10 or 11 trilayer 2.5 mu m 2 Nb-AlO x -Nb junctions. Best values of T r (DSB) as low as 20+or-2 K have been measured at the receiver room temperature horn in the 104-108 GHz LO range with a 4 GHz IF and at a mixer ambient temperature of 4.5-5.5 K. An SSB mixer noise temperature as low as 6+or-3 K was estimated. This value is very close to the quantum noise limit hf/k approximately=5 K.

DOI
10.1088/0953-2048/4/9/006

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IEEE Transactions on Magnetics•Mar 1, 1991•0 citations
The possibility of overcoming the main drawbacks of the traditional series arrays by using a parallel connection of SIS junctions for DC and IF current has been experimentally demonstrated in full height 70-116 GHz waveguide mixers. This new array concept has been successfully developed to: (i) avoid the influence of junction non-uniformity in the array; (ii) provide optimal matching at both RF input and IF output even in the case of high gain, and (iii) tune out junction capacitance without any DC blocks. The experimentally tested arrays contain 10 or 11 trilayer 2.5 mu m 2 Nb-AlO x -Nb junctions. Best values of T r (DSB) as low as 20+or-2 K have been measured at the receiver room temperature horn in the 104-108 GHz LO range with a 4 GHz IF and at a mixer ambient temperature of 4.5-5.5 K. An SSB mixer noise temperature as low as 6+or-3 K was estimated. This value is very close to the quantum noise limit hf/k approximately=5 K.
The possibility of overcoming the main drawbacks of the traditional series arrays by parallel connection of the SIS (superconductor-insulator-superconductor) junctions for DC and IF are demonstrated experimentally. The proposed mixing elements avoid the influence of the junction nonuniformity in the array, provide the optimal matching on both RF input and IF output, and tune out junction capacitance. Experimentally tested arrays contained up to eight high-quality Nb-AlO/sub x/-Nb junctions with R/sub n/=20-70 Omega at junction area 8/14 mu m/sup 2/. The best values of T/sub r/ (SSB) were measured to as low as 5 K on the mixer cold input flange in the 45-55-GHz bandwidth at an ambient temperature of 4.2 K. A mixer gain of up to 10 dB was obtained. The gain values were limited by bias stability at very high or even negative array output impedance. An experimental receiver noise temperature (SSB) of less than 20 K has been achieved.
Parallel connected for dc and IF, but in series for rf current SIS junction arrays are under investigation since 1982. Novel conception of the improved matching for both input and output mixer ports have been developed and confirmed successfully with experimental receivers in 40-180 GHz frequency range. Parallel and parallel-series combinations integrated up to 11 Nb-AlOx-Nb type SIS junctions have been tested in full height waveguide mixers. The receivers' noise temperatures Tr(DSB) I50K have been achieved in the laboratory tests across frequency range 40-150GHz. The Tr as low as 35K have been carefully measured at 145GHz. The parallel biased SIS arrays for integrated on a chip SIS receiver have been designed and tested successfully. The integrated receiver noise temperature as low as 85K was achieved at 140GHz. New SIS array design for mixer in frequency range 500-1000 GHz is presented.
Several SIS quasiparticle mixers have been designed and tested for the frequency range from 80 to 115 GHz. The sliding back short is the only adjustable RF-tuning element. The RF-filter reactance is used a s a fixed RF-matching element. A mixer which uses a single 2 × 2 μm2Pb-alloy junction in a 1/4-height waveguide mount has a coupled conversion gain of GM(DSB) = 2.6 ± 0.5 dB with an associated noise temperature of TM(DSB) = 16.4 ± 1.8 K at the best DSB operation point. The receiver noise temperature TR(DSB) is 27.5 ± 0.8 K for the test apparatus. This mixer provides a SSB receiver noise temperature below 50 K over the frequency range from 91 to 96 GHz, the minimum being TR(SSB) = 44 ± 4 K. Another mixer with an array of five 5 × 5 μm2junctions in series has much lower noise TM(DSB) = 6.6 ± 1.6 K, but less gain GM(DSB) = -5.1 ± 0.5 dB.
This paper reports on the performance of a broadband SIS receiver with no mechanical tuning elements was scale modelled and tested. The mixer mount had a broadband waveguide to microstripline transition consisting of a 4-step Chebychev single ridge transformer. The last step of the ridge connected the waveguide to a microstripline circuit. The on-chip circuit consisted of a microstripline, which transmitted the rf and the local oscillator signals to the SIS mixer. Some chips included a thin film strip inductor in parallel with the 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}(2mV) = 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, we achieved a mixer noise temperature of 35 K at 100 GHz increasing to 45 K at 79.5 andmore » 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.« less