(1996). ГОСТ Р 50995.3.1-96. Технологическое обеспечение создания продукции. Технологическая подготовка производства.
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-. (1996). ГОСТ Р 15.011-96. Патентные исследования. Содержание и порядок проведения.
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Belitsky, V. Y., & Kollberg, E. L. (1996). Tuning circuit for NbN SIS mixer. In Proc. 7th Int. Symp. Space Terahertz Technol. (234). Charlottesville, Virginia, USA.
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Yagubov, P., Gol'tsman, G., Voronov, B., Seidman, L., Siomash, V., Cherednichenko, S., et al. (1996). The bandwidth of HEB mixers employing ultrathin NbN films on sapphire substrate. In Proc. 7th Int. Symp. Space Terahertz Technol. (pp. 290–302). Charlottesville, Virginia, USA.
Abstract: We report on some unusual features observed during fabrication of ultrathin NbN films with high Tc. The films were used to fabricate HEB mixers, which were evaluated for IF bandwidth measurements at 140 GHz. Ultrathin films were fabricated using reactive dc magnetron sputtering with a discharge current source. Reproducible parameters of the films are assured keeping constant the difference between the discharge voltage in pure argon, and in a gas mixture, for the same current. A maximum bandwidth of 4 GHz at optimal LO and dc bias was obtained for mixer chip based on NbN film 35 A thick with Tc = 11 K.
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Kawamura, J., Blundell, R., Tong, C. - Y. E., Golts'man, G., Gershenzon, E., & Voronov B. (1996). Superconductive NbN hot-electron bolometric mixer performance at 250 GHz. In Proc. 7th Int. Symp. Space Terahertz Technol. (pp. 331–336).
Abstract: Thin film NbN (<40 A) strips are used as waveguide mixer elements. The electron cooling mechanism for the geometry is the electron-phonon interaction. We report a receiver noise temperature of 750 K at 244 GHz, with / IF = 1.5 GHz, Af= 500 MHz, and Tphysical = 4 K. The instantaneous bandwidth for this mixer is 1.6 GHz. The local oscillator (LO) power is 0.5 1.tW with 3 dB-uncertainty. The mixer is linear to 1 dB up to an input power level 6 dB below the LO power. We report the first detection of a molecular line emission using this class of mixer, and that the receiver noise temperature determined from Y-factor measurements reflects the true heterodyne sensitivity.
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Hesler, J. L., Hall, W. R., Crowe, T. W., Weikle, R. M., Bradley, R. F., & Pan, S. - K. (1996). Submm wavelenght waveguide mixers using planar Schottky barier diods. In Proc. 7th Int. Symp. Space Terahertz Technol. (462).
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Tong, C. Y. E., Blundell, R., Bumble, B., Stern, J. A., & LeDuc, H. G. (1996). Sub-Millimeter distributed quasiparticle receiver employing a non-Linear transmission line. In Proc. 7th Int. Symp. Space Terahertz Technol. (47).
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Nebosis, R. S., Semenov, A. D., Gousev, Y. P., & Renk, K. F. (1996). Rigorous analysis of a superconducting hot-electron bolometer mixer: theory and comparision with experiment. In Proc. 7th Int. Symp. Space Terahertz Technol. (pp. 601–613). Charlottesville, Virginia, USA.
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Kerr, A. R., Feldman, M. J., & Pan, S. - K. (1996). Receiver noise temperature, the quantum noise limit, and the role of the zero-point fluctuations. Electronics division internal report NO. 304, , 1–10.
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Gousev, Y. P., Gol'tsman, G. N., Karasik, B. S., Gershenzon, E. M., Semenov, A. D., Barowski, H. S., et al. (1996). Quasioptical superconducting hot electron bolometer for submillmeter waves. Int. J. of Infrared and Millimeter Waves, 17(2), 317–331.
Abstract: We report on a superconducting hot electron bolometer coupled to radiation via a broadband antenna. The bolometer, a structured NbN film, was patterned on a thin dielectric membrane between terminals of a gold slotline antenna. We investigated the response to submillimeter radiation (wave-lengths ∼ 0.1 mm to 0.7 mm) in the fundamental Gaussian mode. We found that the directivity of the antenna was constant within a factor of 2.5 through the whole experimental range. The noise equivalent power of the bolometer at 119 µm was ∼ 3 · 10−13 W/Hz1/2; a time constant of ∼ 160 ps was estimated.
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