We have designed, fabricated, and tested the waveguide receiving element, which is based on the tunnel superconductor–insulator–superconductor structures, for the frequency range 790–950 GHz. Two Nb/AlN/NbN tunnel junctions are incorporated in a microstrip line consisting of the bottom NbTiN-film electrode with a thickness of about 300 nm and the top 500 nm-thick aluminum electrode. The production-process optimization allows one to ensure the following characteristics of these junctions: submicron area (0.5 μm2 for each junction), current density about 30 kA/cm2, and band gap width 3.2 mV. Such tunnel junctions ensure the receiver operation in a wide frequency range (700–950 GHz), which was confirmed by the Fourier transform spectroscopy and the noise-temperature measurements. At a frequency of 725 Hz, the corrected noise temperature of the receiver amounts to 120 K, which is only threefold greater than the quantum limit hf/kB, where h is the Planck’s constant, f is the frequency, and kB is Boltzmann’s constant. In the upper part of this frequency range, the noise temperature increases up to 390 K.
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 59, No. 8–9, pp. 793–797, August–September 2016.
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Rudakov, K.I., Koshelets, V.P., Baryshev, A.M. et al. The 700–950 GHz Superconducting Receiving Structures for Radio Astronomy. Radiophys Quantum El 59, 711–714 (2017). https://doi.org/10.1007/s11141-017-9739-5
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DOI: https://doi.org/10.1007/s11141-017-9739-5