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Author Bremer, J. W.; Newhouse, V. L.
Title Type Journal Article
Year 1958 Publication Phys. Rev. Lett. Abbreviated Journal
Volume 1 Issue Pages 282
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Address Bremer, J. W.; Newhouse, V. L.
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Notes Approved no
Call Number MSPU @ s @ bremer_prl_1958 Serial 215
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Author Андреев, А. Ф.
Title Type Journal Article
Year 1964 Publication ЖЭТФ Abbreviated Journal
Volume 46 Issue Pages 1823-1827
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Notes Approved no
Call Number MSPU @ s @ Andreev_reflection_rus Serial 217
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Author Финкель, М. И.; Масленников, С. Н.; Гольцман, Г. Н.
Title Концепция приёмного комплекса космического радиотелескопа «Миллиметрон» Type Journal Article
Year 2007 Publication Известия высших учебных заведений. Радиофизика Abbreviated Journal
Volume 50 Issue 10-11 Pages 924-934
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Language russian Summary Language Original Title
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Call Number RPLAB @ s @ mix_review_2007_rus Serial 410
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Author Ryabchun, S. A.; Tretyakov, I. V.; Finkel, M. I.; Maslennikov, S. N.; Kaurova, N. S.; Seleznev, V. A.; Voronov, B. M.; Goltsman, G. N.
Title Fabrication and characterisation of NbN HEB mixers with in situ gold contacts Type Conference Article
Year 2008 Publication Proc. 19th Int. Symp. Space Terahertz Technol. Abbreviated Journal Proc. 19th Int. Symp. Space Terahertz Technol.
Volume Issue Pages 62-67
Keywords HEB, mixer, NbN, in-situ contacts
Abstract We present our recent results of the fabrication and testing of NbN hot-electron bolometer mixers with in situ gold contacts. An intermediate frequency bandwidth of about 6 GHz has been measured for the mixers made of a 3.5-nm NbN film on a plane Si substrate with in situ gold contacts, compared to 3.5 GHz for devices made of the same film with ex situ gold contacts. The increase in the intermediate frequency bandwidth is attributed to additional diffusion cooling through the improved contacts, which is further supported by the its dependence on the bridge length: intermediate frequency bandwidths of 3.5 GHz and 6 GHz have been measured for devices with lengths of 0.35 μm and 0.16 μm respectively at a local oscillator frequency of 300 GHz near the superconducting transition. At a local oscillator frequency of 2.5 THz the receiver has offered a DSB noise temperature of 950 K. When compared to the previous result of 1300 K obtained at the same local oscillator frequency for devices fabricated with an ex situ route, such a low value of the noise temperature may also be attributed to the improved gold contacts.
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Publisher Place of Publication Groningen, Netherlands Editor
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Call Number Serial 412
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Author Yagoubov, P.; van de Stadt, H.; Hoogeveen, R.; Koshelets, V.; Birk, Manfred; Murk, A.
Title OPTICAL DESIGN OF SUB-MILLIMETER SPECTROMETER FOR LIMB SOUNDER Type Journal Article
Year 2005 Publication International Symposium on Space Terahertz Technology Abbreviated Journal
Volume Issue Pages
Keywords Cryogenic terahertz heterodyne receiver, remote sensing, TELIS, submillimeter
Abstract TELIS (Terahertz and submm Limb Sounder) is a cooperation between DLR (Institute for Remote Sensing Technology, Germany), RAL (Rutherford Appleton Laboratories, UK) and SRON (National Institute for Space Research, the Netherlands), to build a three-channel balloon-borne heterodyne spectrometer for atmospheric research. The three receivers will operate simultaneously at 500 GHz (channel developed by RAL), at 550-650 GHz (SRON in collaboration with IREE), and at 1.8 THz (DLR). The balloon platform on which TELIS will fly also contains a Fourier transform spectrometer: MIPAS-B developed by the IMK (Institute of Meteorology and Climate research of the University of Karlsruhe, Germany). MIPAS-B will simultaneously measure within the range 680 to 2400 cm-1. The combination of the TELIS and MIPAS instruments will provide an unprecedented wealth of scientific data and will also be used to validate other instruments and atmospheric chemistry models. In this paper we present the optical design of TELIS with an emphasis on the 550-650 GHz channel. The main design goal was to generate a high efficiency antenna beam over the full frequency range, with low side lobes and close to diffraction limited angular resolution in the vertical direction at the sky. All these requirements had to be achieved within a small volume and low mass. Design and validation of the optics, as well as estimation of optical components tolerances, was done using commercial software packages ZEMAX and GRASP.
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Notes event_dates=2005-05-31 – 2005-06-03; Approved no
Call Number Serial 414
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