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Nebosis RS, Semenov AD, Gousev YP, Renk KF. Rigorous analysis of a superconducting hot-electron bolometer mixer: theory and comparision with experiment. In: Proc. 7th Int. Symp. Space Terahertz Technol. Charlottesville, Virginia, USA; 1996. p. 601–13.
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-. ГОСТ Р 15.011-96. Патентные исследования. Содержание и порядок проведения.; 1996.
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ГОСТ Р 50995.3.1-96. Технологическое обеспечение создания продукции. Технологическая подготовка производства.; 1996.
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Kawamura J, Blundell R, Tong C-YE, Golts'man G, Gershenzon E, Voronov B. Superconductive NbN hot-electron bolometric mixer performance at 250 GHz. In: Proc. 7th Int. Symp. Space Terahertz Technol.; 1996. p. 331–6.
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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Kerr AR, Feldman MJ, Pan S-K. Receiver noise temperature, the quantum noise limit, and the role of the zero-point fluctuations. Electronics division internal report NO. 304. 1996:1–10.
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