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http://www.issp.ac.ru/lhpp/PapersAntonov/122.pdf.
http://www.issp.ac.ru/lhpp/PapersAntonov/122.pdf.
1. http://www.issp.ac.ru/lhpp/PapersAntonov/138e.pdf
... 76, No. 5, 2002, pp. ... Hydrogen Tunneling Modes in a-Mn Suppressed by Elastic Stresses V. E. Antonov1, V. P. Glazkov2, *, D. P. Kozlenko3, B. N. Savenko3, V. A. Somenkov2, and V. K. Fedotov1 1 Institute of Solid State ... 142432 Russia 2 Russian Research Centre Kurchatov Institute, Moscow, 123182 Russia * e-mail: glazkov@isssph.kiae.ru 3 Laboratory of Neutron Physics, Joint Institute for Nuclear Research, Dubna, Moscow region, 141980 Russia Received August 6, 2002 Behavior of the ...
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Ссылки http://www.issp.ac.ru/lhpp/PapersAntonov/138e.pdf -- 49.8 Кб -- 10.02.2012
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2. http://www.cplire.ru/html/lab234/pubs/2005-23.pdf
TOWARDS SUPERSENSITIVE BOLOMETERS AND ELECTRON COOLERS BASED ON CARBON NANOTUBES M.TARASOV, J.SVENSSON, S.DITTMER, L.KUZMIN, AND E.CAMPBELL Chalmers University of Technology, GЖteborg SE 41294, Sweden E-mail: Mikhail.tarasov@mc2.chalmers.se Carbon nanotubes (CNT) are being intensively developed for novel electronics. Electron cooling by superconductor-insulator-nanotube (SIN) tunnel junctions could be extremely effective due to the small volume of the CNT. ...
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Ссылки http://www.cplire.ru/html/lab234/pubs/2005-23.pdf -- 253.5 Кб -- 24.01.2006
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3. The AO Optical Laboratories National Astronomy and Ionosphere Center (Arecibo
NATIONAL ASTRONOMY AND IONOSPHERE CENTER . ... Astronomy . ... Visitor Center . ... Optical . Lidar . At Arecibo we have a variety of optical instruments that we use to study terrestrial airglow emissions. ... This equipment is located in our Optical Laboratory, which is on site about 1000 feet from the center of the incoherent scatter radar. ... The various observational modes that are available are described in supplementary documentation for the Arecibo Observatory Optical Laboratories. ...
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Ссылки http://www.naic.edu/general/index.php?option=com_content&view=article&id=173:atmos-optical&catid=109&Itemid=476 -- 22.0 Кб -- 13.04.2016
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4. Time Tunnel
Astronomy Picture of the Day . ... Spanning about 1/2 degree on the sky, the pretty picture is the result of astronomer Johannes Schedler's project to look back in time, toward a quasar 12.7 billion light-years away . ... Of course, the expansion of the Universe has redshifted the light. Schedler added image data extending to the near-infrared, acquired by collaborator Ken Crawford, to detect the distant quasar, with a measured redshift of 6.04. ... Publications with keywords: quasar - redshift . ...
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Ссылки http://www.astronet.ru/db/xware/msg/1223380 -- 15.3 Кб -- 06.09.2007
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5. Fabrication Technology for Single Electron Transistors and Submillimeter
... We describe efforts to develop a robust fabrication technology for making submillimeter detectors integrated with single electron transistors as readout amplifiers. ... Thus, the RF-SET can amplify the small photocurrent generated in a superconducting tunnel junction detector by a single submillimeter photon. ... The antenna, detector, and SET are contained in 4 fields, which are fabricated with electron beam lithography and Al double angle evaporation techniques. ... FABRICATION OF SQPC CHIP . ...
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Ссылки http://www.stsci.edu/stsci/meetings/space_detectors/x-band.htm -- 17.6 Кб -- 30.08.2001
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6. APOD: 2007 September 6 - Time Tunnel
... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2007 September 6 . Time Tunnel . ... Spanning about 1/2 degree on the sky, the pretty picture is the result of astronomer Johannes Schedler's project to look back in time, toward a quasar 12.7 billion light-years away . ... The quasar appears as it did about 12.7 billion years ago, when the Universe was just 7 percent of its present age . ...
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Ссылки http://www.sai.msu.su/apod/ap070906.html -- 5.4 Кб -- 02.10.2012
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7. The AstroStat Slog emission measure
... Posts tagged ?emission measure? ... Spectral lines are a ubiquitous feature of astronomical data. ... Continue reading ?Line Emission [EotW]? Tags: abundance , emission , emission measure , emissivity , EotW , Equation , Equation of the Week , flux , ion balance , line . ... 2 Comments . ... Entries RSS . ... vlk on [MADS] Parallel Coordinates . upvc windows on [MADS] Parallel Coordinates . ... Alfred Inselberg on [MADS] Parallel Coordinates . ... Entries (RSS) and Comments (RSS) . ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/tag/emission-measure/index.html -- 19.6 Кб -- 01.03.2014
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8. Optical instrumentation [Oulu]
... Despite new observation methods provided by radar and satellite instrumentation , optical measurements are still important when studying auroras . ... Because of the monochromatic nature of the auroral light, photomultiplier tubes with very narrow band filters were used in the measurements. ... The spectra of the background emissions from atmospheric impurities (clouds, ice crystals, etc.) is rather continuous, and measurements just outside the auroral emission lines are valid for the line itself. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/optical.html -- 4.2 Кб -- 21.12.2007
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9. INFRARED FOURIER-SPECTROMETER SICH-F
INFRARED FOURIER-SPECTROMETER SICH-F . ... Instrument work regimes: 1) Inside. 2) Calibration at inside standard sources 2 - 4 times per a rotation. 3) Calibration at "free space" 2 - 4 times per a rotation. 4) Infrared radiation measuring 10 - 40 min. per a rotation. ... Spectrometer consists of the photodetector block and the block of signal processing and control. ... Diagnostic information and attach data will transfer by state telemetric channels. ... Detector temperature. ...
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Ссылки http://space.univ.kiev.ua/projects/warning/sich.html -- 7.5 Кб -- 15.02.2000
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10. The errors in the measured off-sets
. XMM-Newton Science Analysis System . eposcorr (eposcorr-3.12) [xmmsas_20070708_1801-7.1.0] . Meta Index / Home Page / Description At the moment we have no rigurous mathematical method to handle the statistical errors of the offsets found. For the moment we use the square root of the second order moment in as a function of off-set divided by the number of optical counter parts. XMM-Newton SOC/SSC -- 2007-07-08
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Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/eposcorr/node5.html -- 3.5 Кб -- 08.07.2007