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Tinkham M. Introduction to superconductivity. 2nd ed. USA; 1996.
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Currie NC, Demma FJ, Ferris Jr. DD, Kwasowsky BR, McMillan RW, Wicks MC. Infrared and millimeter-wave sensors for military special operations and law enforcement applications. Int. J. Infrared and Millimeter Waves. 1996;17(7):1117–38.
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Dickert FL, Haunschild A, Kuschow V, Reif M, Stathopulos H. Mass-sensitive detection of solvent vapors. Mechanistic studies on host-guest sensor principles by FT-IR spectroscopy and BET adsorption analysis. Anal Chem. 1996;68(6):1058–61.
Abstract: Chemical sensors, based on highly mass sensitive QMB or SAW devices, coated with thin layers of calixarenes, enable the detection of organic solvent vapours, especially halogenated or aromatic hydrocarbons, down to a few ppm. Force field calculations allow the tailoring of these sensor materials seeing that the predicted interaction energies between the host molecules and a large variety of analytes are linearly correlated to the measured sensor effects. These correlations and also BET adsorption analysis prove the analyte recognition properties of these calixarene coatings to be mainly based on host/guest inclusion principles.
Keywords: supramolecular recognition, quartz crystal microbalance, QCM, surface acoustic wave, SAW, mass-sensitive sensor, detector, calixarenes, MM3 force field, Brunauer, Emmett and Teller theory, BET
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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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Gousev YP, Semenov AD, Pechen EV, Varlashkin AV, Nebosis RS, Renk K. F. Coupling of terahertz radiation to a high-Т(с) superconducting hot electron bolometer mixer. Appl Phys Lett,. 1996;69:691–3.
Abstract: We report on efficient coupling of THz radiation to a high-T(c) superconducting hot electron bolometer that is suitable for heterodyne detection. Our quasioptical system consisted of a planar self-complementary spiral antenna on a dielectric substrate clamped to an extended hyperhemispherical lens. The antenna was integrated into a co-planar line for broadband intermediate frequency matching. Measurements in the homodyne regime at a frequency of 2.5 THz showed a radiation pattern with a beam width of 1° and a coupling efficiency of 0.1. We measured, at an intermediate frequency of 1.5 GHz, an output noise temperature of'160 K and estimated for the device, operated in the heterodyne regime, a system noise temperature of 30 000 K. We also discuss possibilities of significant improvement of the sensitivity.
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Ekström H, Kroug M, Belitsky V, Kollberg E, Olsson H, Goltsman G, et al. Hot electron mixers for THz applications. In: Rolfe EJ, Pilbratt G, editors. Proc. 30th ESLAB.; 1996. p. 207–10.
Abstract: We have measured the noise performance of 35 A thin NbN HEB devices integrated with spiral antennas on antireflection coated silicon substrate lenses at 620 GHz. From the noise measurements we have determined a total conversion gain of the receiver of—16 dB, and an intrinsic conversion of about-10 dB. The IF bandwidth of the 35 A thick NbN devices is at least 3 GHz. The DSB receiver noise temperature is less than 1450 K. Without mismatch losses, which is possible to obtain with a shorter device, and with reduced loss from the beamsplitter, we expect to achieve a DSB receiver noise temperature of less ‘than 700 K.
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