Zobrazeno 1 - 10
of 24
pro vyhledávání: '"V. G. Rodin"'
Publikováno v:
Measurement Techniques. 65:432-437
Autor:
D. S. Goncharov, E. K. Petrova, T. Sh. Fazliev, V. G. Rodin, N. A. Trocenko, Rostislav S. Starikov, N. M. Ponomarev
Publikováno v:
Radiophysics and Quantum Electronics. 63:605-611
We present the results of simulation of image recognition using invariant correlation filters. The possibilities of exploiting color information and preprocessing for quality improvement of subpixel image correlation matching are shown.
Autor:
P. А. Dukanov, V. G. Rodin, А. I. Grushin, Nikolay N. Prokopenko, Dmitry G. Drozdov, E. M. Savchenko
Publikováno v:
Visnyk NTUU KPI Seriia-Radiotekhnika Radioaparatobuduvannia; 79; 71-77
Вестник НТУУ" КПИ ". Серия радиотехника Радиоаппаратостроение; 79; 71-77
Вісник НТУУ "КПІ". Серія Радіотехніка, Радіоапаратобудування; 79; 71-77
Вісник НТУУ «КПІ». Радіотехніка, радіоапаратобудування: збірник наукових праць, Вип. 79
Вестник НТУУ" КПИ ". Серия радиотехника Радиоаппаратостроение; 79; 71-77
Вісник НТУУ "КПІ". Серія Радіотехніка, Радіоапаратобудування; 79; 71-77
Вісник НТУУ «КПІ». Радіотехніка, радіоапаратобудування: збірник наукових праць, Вип. 79
We have developed technology and construction solutions system to increase differential pairs (DP) of JFet with p- and n-channels identity, which are included into silicon complementary bipolar process of SPE “Pulsar” (Moscow). The possibility of
Autor:
V. G. Rodin
Publikováno v:
Компьютерная оптика, Vol 42, Iss 3, Pp 347-353 (2018)
The possibility of application of a digital micromirror device (DMD) as a spatial light modulator for outputting holographic filters in an optical correlator illuminated by quasi-monochromatic spatially incoherent radiation was discussed. The experim
Autor:
V. Bonvicini, A. M. Galper, O. F. Prilutskii, N. Zampa, Mirko Boezio, A. L. Menshenin, M. I. Fradkin, E. P. Mazets, V. G. Zverev, V. G. Rodin, V. A. Kachanov, N. P. Topchiev, Piero Spillantini, V. A. Kaplin, I V Arkhangelskaya, B. A. Dolgoshein, S. I. Suchkov, A. Vacchi, Yu. T. Yurkin, R. L. Aptekar, V. Ya. Gecha, M. F. Runtso, P. Picozza, M. O. Farber
Publikováno v:
Astrophysics and Space Sciences Transactions. 7:75-78
The GAMMA-400 space observatory will pro- vide precise measurements of gamma rays, electrons, and positrons in the energy range 0.1-3000 GeV. The good an- gular and energy resolutions, as well as identification capa- bilities (angular resolution 0.01
Autor:
S. I. Suchkov, Andrea Vacchi, Francesco Longo, Roberta Sparvoli, Piero Spillantini, Yu. T. Yurkin, M. F. Runtso, P. Yu. Naumov, N. Zampa, O. Adriani, Vladimir Kaplin, E. Vannuccini, M. D. Kheymits, V. G. Zverev, A. A. Leonov, Yu. V. Gusakov, R. L. Aptekar, E. Mocchiutti, A. A. Moiseev, P. Papini, Igor V. Moskalenko, P S Marrocchesi, K. A. Boyarchuk, I. V. Arkhangelskaja, V. A. Kachanov, V. G. Rodin, P. Picozza, Nicola Mori, E. P. Mazets, A. M. Galper, V. Bonvicini, M. I. Fradkin, Marco Tavani, Mirko Boezio, N. P. Topchiev, Paolo Maestro, M. O. Farber, A.I. Arkhangelskiy
The preliminary design of the new space gamma-ray telescope GAMMA-400 for the energy range 100 MeV - 3 TeV is presented. The angular resolution of the instrument, 1-2{\deg} at E{\gamma} ~100 MeV and ~0.01^{\circ} at E{\gamma} > 100 GeV, its energy re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da2958525f777eb8b7ecbf02ff3f0ff0
http://hdl.handle.net/11368/2710482
http://hdl.handle.net/11368/2710482
Autor:
P. Spillantini, N. Zampa, Ritabrata Sarkar, K. A. Boyarchuk, Igor V. Moskalenko, Ps Marrocchesi, A. A. Leonov, I. V. Arkhangelskaja, Nicola Mori, Andrea Vacchi, I. A. Mereminskiy, V. Bonvicini, A. A. Moiseev, Francesco Longo, V. G. Rodin, R. L. Aptekar, Roberta Sparvoli, P. Picozza, E. P. Mazets, P. Papini, Yu. V. Gusakov, E. Vannuccini, M. F. Runtso, Yu. T. Yurkin, O. Adriani, V. A. Kachanov, V. N. Zirakashvili, E. Mocchiutti, P. Cumani, V. G. Zverev, R. Carbone, A.I. Arkhangelskiy, V. V. Mikhailov, M. D. Kheymits, S. I. Suchkov, Mirko Boezio, N. P. Topchiev, Paolo Maestro, A. M. Galper, M. I. Fradkin, Marco Tavani, P. Yu. Naumov, Vladimir Kaplin
The present design of the new space gamma-ray telescope GAMMA-400 for the energy range 50 MeV–3 TeV is presented. The proposed instrument has an angular resolution of 1–2 degrees at E(gamma)~100 MeV and ∼0.01 degrees at E(gamma)>100 GeV and an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cbceeb5827622555727ca6c764900bf0
https://hdl.handle.net/11368/2710484
https://hdl.handle.net/11368/2710484
Autor:
P. B. Price, V. G. Afanasyev, L. A. Gorshkov, Andrew J. Westphal, V. G. Rodin, N.A.C Gunn, V. V. Akimov, O. S. Tsigankov, K Baryshnikov, N. I. Shvets
Publikováno v:
Advances in Space Research. 19:743-746
In 1991, the Berkeley-IKI Trek detectors, consisting of stacks of BP-1 track-etch glass, were deployed on the Russian space station Mir. Trek consists of two distinct instruments: one, with the goal of the measurement of the isotopic abundances of ir
Autor:
A. Vacchi, K. A. Boyarchuk, Yu. V. Gusakov, P. Spillantini, M. F. Runtso, F. Longo, E. Mocchiutti, M. D. Kheymits, Nicola Mori, V. Bonvicini, I. V. Arkhangelskaja, I. A. Mereminskiy, V. G. Rodin, N. Zampa, S. I. Suchkov, A. A. Moiseev, E. P. Mazets, O. Adriani, P. Picozza, V. A. Kaplin, V. A. Kachanov, A. A. Leonov, R. L. Aptekar, Roberta Sparvoli, P. S. Marrocchesi, V. V. Mikhailov, V. G. Zverev, Igor V. Moskalenko, N. P. Topchiev, Paolo Maestro, A.I. Arkhangelskiy, Mirko Boezio, Y. T. Yurkin, A. M. Galper, P. Yu. Naumov, P. Papini, E. Vannuccini, V. N. Zirakashvili, M. I. Fradkin, Marco Tavani
The GAMMA-400 gamma-ray telescope currently under development is designed to measure fluxes of gamma rays and electron-positron cosmic-ray components, which could be associated with the annihilation or decay of dark matter particles, and to survey in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f7377213eee0460f411af340524782e6
http://hdl.handle.net/11390/1126691
http://hdl.handle.net/11390/1126691
Publikováno v:
Quantum Electronics. 25:1014-1019
A description is given of systems with spatially incoherent illumination, intended for spectral and correlation analysis, and for the recording of Fourier holograms. These systems make use of transformation of the degree of the spatial coherence of l