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Author Dahl, H.; Metz, H. J.; Wriedt, T.
Title Light scattering of silver halide crystals Type Conference Article
Year 1998 Publication Proc. 3rd Workshop on Electromagnetic and Light Scattering Abbreviated Journal
Volume Issue Pages 51-58
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Publisher Place of Publication Universität Bremen Editor
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Notes Approved no
Call Number Serial 504
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Author Bingham, S. J.; Börger, B.; Suter, D.; Thomson, A. J.
Title The design and sensitivity of microwave frequency optical heterodyne receivers Type Journal Article
Year 1998 Publication Review of Scientific Instruments Abbreviated Journal Rev. Sci. Instrum.
Volume 69 Issue 9 Pages 3403-3409
Keywords optical mixing
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ISSN 0034-6748 ISBN Medium
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Notes Approved no
Call Number Serial 508
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Author Dieleman, Piter
Title Fundamental limitations of THz niobium and niobiumnitride SIS mixers Type Book Whole
Year 1998 Publication Abbreviated Journal
Volume Issue Pages
Keywords SIS
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Corporate Author Thesis Ph.D. thesis
Publisher Place of Publication Rijksuniversiteit, Groningen Editor
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Notes Approved no
Call Number Serial 529
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Author Kawamura, Jonathan; Blundell, Raymond; Tong, C.-Y. Edward; Papa, D. Cosmo; Hunter, Todd R.; Gol'tsman, Gregory; Cherednichenko, Sergei; Voronov, Boris; Gershenzon, Eugene
Title First light with an 800 GHz phonon-cooled HEB mixer receiver Type Conference Article
Year 1998 Publication Proc. 9th Int. Symp. Space Terahertz Technol. Abbreviated Journal Proc. 9th Int. Symp. Space Terahertz Technol.
Volume Issue Pages 35-43
Keywords HEB, mixer, LO power, local oscillator power, saturation effect, dynamic range
Abstract Phonon-cooled superconductive hot-electron bolometric (HEB) mixers are incorporated in a waveguide receiver designed to operate near 800 Gliz. The mixer elements are thin-film nio- bium nitride microbridges with dimensions of 4 nm thickness, 0.2 to 0.3 p.m in length and 2 jun in width. At 780 GHz the best receiver noise temperature is 840 K (DSB). The mixer IF bandwidth is 2.0 GHz, the absorbed LO power is —0.1 1.1W. A fixed-tuned version of the re- ceiver was installed at the Submillimeter Telescope Observatory on Mt. Graham, Arizona, to conduct astronomical observations. These observations represent the first time that a receiver incorporating any superconducting HEB mixer has been used to detect a spectral line of celes- tial origin.
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Publisher Place of Publication Pasadena, California, USA Editor
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Notes Approved no
Call Number Serial 572
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Author Burke, P. J.; Schoelkopf, R. J.; Prober, D. E.; Skalare, A.; Karasik, B. S.; Gaidis, M. C.; McGrath, W. R.; Bumble, B.; Leduc, H. G.
Title Spectrum of thermal fluctuation noise in diffusion and phonon cooled hot-electron mixers Type Journal Article
Year 1998 Publication Applied Physics Letters Abbreviated Journal Appl. Phys. Lett.
Volume 72 Issue 12 Pages 1516-1518
Keywords HEB mixer; thermal fluctuation noise; TFN
Abstract A systematic study of the intermediate frequency noise bandwidth of Nb thin-film superconducting hot-electron bolometers is presented. We have measured the spectrum of the output noise as well as the conversion efficiency over a very broad intermediate frequency range (from 0.1 to 7.5 GHz) for devices varying in length from 0.08 μm to 3 μm. Local oscillator and rf signals from 8 to 40 GHz were used. For a device of a given length, the spectrum of the output noise and the conversion efficiency behave similarly for intermediate frequencies less than the gain bandwidth, in accordance with a simple thermal model for both the mixing and thermal fluctuation noise. For higher intermediate frequencies the conversion efficiency decreases; in contrast, the noise decreases but has a second contribution which dominates at higher frequency. The noise bandwidth is larger than the gain bandwidth, and the mixer noise is low, between 120 and 530 K (double side band).
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Notes Approved no
Call Number RPLAB @ gujma @ Serial 760
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