2,581 research outputs found

    РаспознаваниС ΠΈΠ·ΠΎΠ±Ρ€Π°ΠΆΠ΅Π½ΠΈΠΉ Π»ΠΈΡ† Π½Π° основС кластСризации

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    This article describes the use of clustering for face recognition image. Clustering was performed using a recurrent neural network used at two stages of the recognition process. The algorithm includes the recognition process itself perform clustering pixel brightness image, calculating image information close proximity and clustering measures to in order to obtain the cluster containing the original similar images

    ΠŸΡ€ΠΈΠ±ΠΎΡ€ для измСрСния ΠΏΠ°Ρ€Π°ΠΌΠ΅Ρ‚Ρ€ΠΎΠ² ΠΌΠ°Π³Π½ΠΈΡ‚ΠΎΠΏΡ€ΠΎΠ²ΠΎΠ΄Π° Π±Π΅Ρ‚Π°Ρ‚Ρ€ΠΎΠ½Π°

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    Π’ Π΄Π°Π½Π½ΠΎΠΉ выпускной ΠΊΠ²Π°Π»ΠΈΡ„ΠΈΠΊΠ°Ρ†ΠΈΠΎΠ½Π½ΠΎΠΉ Ρ€Π°Π±ΠΎΡ‚Π΅ рассмотрСн способ контроля ΠΏΠ°Ρ€Π°ΠΌΠ΅Ρ‚Ρ€ΠΎΠ² Ρ†Π΅Π½Ρ‚Ρ€Π°Π»ΡŒΠ½Ρ‹Ρ… Π²ΠΊΠ»Π°Π΄Ρ‹ΡˆΠ΅ΠΉ ΠΌΠ°Π»ΠΎΠ³Π°Π±Π°Ρ€ΠΈΡ‚Π½ΠΎΠ³ΠΎ Π±Π΅Ρ‚Π°Ρ‚Ρ€ΠΎΠ½Π°. На основании тСорСтичСских Π΄Π°Π½Π½Ρ‹Ρ… ΠΈ ΡΠΊΡΠΏΠ΅Ρ€ΠΈΠΌΠ΅Π½Ρ‚Π°Π»ΡŒΠ½ΠΎ ΠΏΠΎΠ»ΡƒΡ‡Π΅Π½Π½Ρ‹Ρ… зависимостСй Π±Ρ‹Π» Ρ€Π°Π·Ρ€Π°Π±ΠΎΡ‚Π°Π½ ΠΏΡ€ΠΈΠ±ΠΎΡ€, ΠΏΠΎΠ·Π²ΠΎΠ»ΡΡŽΡ‰ΠΈΠΉ ΠΎΡ†Π΅Π½ΠΈΠ²Π°Ρ‚ΡŒ качСство изготовлСния Ρ†Π΅Π½Ρ‚Ρ€Π°Π»ΡŒΠ½Ρ‹Ρ… Π²ΠΊΠ»Π°Π΄Ρ‹ΡˆΠ΅ΠΉ магнитопроводящСй систСмы Π±Π΅Ρ‚Π°Ρ‚Ρ€ΠΎΠ½Π°. Π’ основС ΠΏΡ€ΠΈΠ½Ρ†ΠΈΠΏΠ° Ρ€Π°Π±ΠΎΡ‚Ρ‹ ΠΏΡ€ΠΈΠ±ΠΎΡ€Π° Π»Π΅ΠΆΠΈΡ‚ способ ΠΎΠΏΡ€Π΅Π΄Π΅Π»Π΅Π½ΠΈΠ΅ добротности ΠΊΠΎΠ»Π΅Π±Π°Ρ‚Π΅Π»ΡŒΠ½ΠΎΠ³ΠΎ ΠΊΠΎΠ½Ρ‚ΡƒΡ€Π° ΠΏΠΎ скорости затухания Π΅Π³ΠΎ элСктричСских ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΠΉ.The method of controlling the parameters of the central inserts block of a betatron was considered in this final qualifying work. The device, which can measure the quality of manufacturing of central inserts block of the magnetic system of the betatron, was developed on the basis of theoretical data and experimentally obtained dependences. The principle of operation of the device is based on the method for determining the quality factor of an oscillating circuit in terms of the rate of damping of its electric oscillations

    Low Voltage Control for the Liquid Argon Hadronic End-Cap Calorimeter of ATLAS

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    At the ATLAS detector a SCADA system surveys and controls the sub- detectors. The link is realized by PVSS2 software and a CanBus hardware system. The low voltages for the Hadronic Endcaps of the liquid argon calorimeter are produced by DC/DC-converters in the power boxes and split into 320 channels corresponding to the pre- amplifier and summing boards in the cryostat. Six units of a prototype distribution board are currently under test. Each of it contains 2 ELMBs as CanBus interface, a FPGA of type QL3012 for digital control and 30 low voltage regulators for the individual fine adjustments of the outputs

    Activation in the COMPTEL double-scattering gamma-ray telescope

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    Abstract-The COMPTEL gamma-ray telescope has been operating in low Earth orbit for six years, since the launch of the Compton Gamma-Ray Observatory in April 1991. Comparisons of data for different orbits and epochs show evidence of activation on time scales from minutes (27Mg, q,2=9.5 min) to years C2Na, q&.58 yr). The activation is correlated with both the orbital altitude and solar cosmic-ray modulation. Because it requires coincident measurements in two different detectors, COMPTEL is most susceptible to instrumental background events in which two or more photons are produced simultaneously

    COMPTEL 1.8 MeV all sky survey: The Cygnus region

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    We present an updated version of COMPTEL’s 1.809 MeV sky survey. Based on eight years of observations we compare results from different imaging techniques using background from adjacent energy bands. We confirm the previously reported characteristics of the galactic 1.809 MeV emission, specifically an extended galactic ridge emission, mainly concentrated towards the inner galaxy, a peculiar emission feature in the Cygnus region, and a low-intensity ridge extending towards Carina and Vela. Because this gamma ray line is due to the decay of radioactive 26Al, predominantly synthesized in massive stars, one anticipates flux enhancements aligned with regions of recent star formation. This is born out by the observations. In particular the Cygnus feature, first presented in 1996 based on three years of COMPTEL data, is confirmed. Based on the stellar population we distinguish three prominent areas in this region, for which we separately derive fluxes, and discuss interpretations
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