Zobrazeno 1 - 10
of 47
pro vyhledávání: '"Yu. V. Gusakov"'
Autor:
D. Yu. Akimov, I. S. Aleksandrov, V. A. Belov, A. I. Bolozdynya, A. A. Vasin, A. V. Galavanov, Yu. V. Gusakov, A. G. Kovalenko, E. S. Kozlova, A. M. Konovalov, V. N. Kornoukhov, A. V. Kumpan, A. V. Luk’yashin, A. V. Pinchuk, O. E. Razuvaeva, D. G. Rudik, G. E. Simakov, V. V. Sosnovtsev, A. V. Khromov, A. V. Shakirov, A. V. Etenko
Publikováno v:
Instruments and Experimental Techniques. 66:199-206
Autor:
G. E. Simakov, V. N. Kornoukhov, A. V. Lukyashin, A.V. Etenko, V.V. Sosnovtsev, D. Yu. Akimov, O. Razuvaeva, A. A. Vasin, Alexander Bolozdynya, V. Belov, A. G. Kovalenko, D. Rudik, A. V. Kumpan, E. S. Kozlova, I. S. Aleksandrov, D.V. Gouss, A. M. Konovalov, D. E. Kdib, A. V. Pinchuk, A. Shakirov, Yu. V. Gusakov, A.V. Khromov, Yu. Efremenko, A. A. Kozlov, A. V. Galavanov
Publikováno v:
Instruments and Experimental Techniques. 64:202-208
A combined passive shield of the RED-100 two-phase emission neutrino detector has been developed and built for suppressing the background of external γ rays and neutrons. The shield is composed of a 5‑cm-thick copper layer (the inner layer is adja
Autor:
Alexey Leonov, A. M. Galper, Yu. V. Gusakov, A. V. Bakaldin, Yu. T. Yurkin, A. E. Egorov, O. D. Dalkarov, N. P. Topchiev, Irina V. Chernysheva, Yu. I. Stozhkov, M. F. Runtso, S. I. Suchkov, A. I. Arkhangelskiy, N. Yu. Pappe, I. V. Arkhangelskaja, M. D. Kheymits
Publikováno v:
Physics of Atomic Nuclei. 83:252-257
The GAMMA-400 gamma-ray telescope is planned for the launch at the end of 2026 on the Navigator service platform designed by Lavochkin Association on an elliptical orbit with following initial parameters: an apogee $${\sim}$$ 300 000, a perigee $${\s
Autor:
Yu. T. Yurkin, I. V. Arkhangelskaja, Yu. I. Stozhkov, O. D. Dalkarov, M. F. Runtso, A. I. Arkhangelskiy, Alexey Leonov, Yu. V. Gusakov, M. D. Kheymits, S. I. Suchkov, A. E. Egorov, A. M. Galper, E. N. Chasovikov, A. V. Bakaldin, Irina V. Chernysheva, N. P. Topchiev, N. Yu. Pappe
Publikováno v:
Physics of Atomic Nuclei. 82:845-854
The GAMMA-400 (Gamma Astronomical Multifunctional Modular Apparatus) will be a new generation satellite gamma-observatory. The gamma-ray telescope GAMMA-400 consists of the anticoincidence system (top and lateral sections—ACtop and AClat), the conv
Autor:
A.M. Konovalov, D. G. Rudik, V.V. Sosnovtsev, A.V. Khromov, O. E. Nepochataya, A. V. Galavanov, A. V. Lukyashin, E. Kozlova, Yu. V. Gusakov, D. Yu. Akimov, D. E. Kdib, A. A. Vasin, A. G. Kovalenko, Alexander Bolozdynya, A. Shakirov, A. V. Kumpan, V. Belov, Yu.A. Melikyan, G. Simakov
Publikováno v:
Instruments and Experimental Techniques. 62:457-463
An integral method is described for processing xenon used as a working medium in the RED-100 two-phase emission detector constructed in the NRNU MEPhI to study the process of elastic coherent neutrino scattering off atomic nuclei. The developed techn
Autor:
S. I. Suchkov, I. V. Arkhangelskaja, N. P. Topchiev, E. N. Chasovikov, A. V. Bakaldin, A. I. Arkhangelskiy, V. G. Zverev, N. Yu. Pappe, Yu. I. Stozhkov, Irina V. Chernysheva, A. E. Egorov, Alexey Leonov, A. M. Galper, M. F. Runtso, Yu. V. Gusakov, O. D. Dalkarov, M. D. Kheymits, Yu. T. Yurkin
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 83:625-628
The GAMMA-400 space project is one of the new generation of space observatories designed to search for signs of dark matter in the cosmic gamma emission, and to measure the characteristics of diffuse gamma-ray emission and gamma-rays from the Sun dur
Autor:
Irina V. Chernysheva, A. V. Bakaldin, A. M. Galper, Yu. T. Yurkin, Yu. I. Stozhkov, O. D. Dalkarov, N. P. Topchiev, Alexey Leonov, M. D. Kheimitz, M. F. Runtso, V. G. Zverev, I. V. Arkhangelskaja, Yu. V. Gusakov, P. Yu. Naumov, N. Yu. Pappe, A. I. Arkhangelskiy, S. I. Suchkov, A. E. Egorov
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 83:629-631
The future space-based γ-ray telescope GAMMA-400 will be installed on the Navigator platform of the Russian astrophysical observatory. A highly elliptical orbit will allow prolonged (~100 days) continuous observations of many regions of the celestia
Autor:
Alexey Leonov, Yu. T. Yurkin, O. D. Dalkarov, N. P. Topchiev, P. Yu. Naumov, Yu. V. Gusakov, S. I. Suchkov, I. V. Arkhangelskaja, A.I. Arkhangelskiy, A. M. Galper, M. D. Kheymits, V. G. Zverev, A. E. Egorov, A. V. Bakaldin, V. V. Kadilin, M. F. Runtso
Publikováno v:
Physics of Atomic Nuclei. 80:1141-1145
The GAMMA-400 γ-ray telescope installed at the Russian space observatory is intended for precision measurements in the energy range of 20 MeV–1000 GeV of γ-ray emission (with the angular and energy resolutions several times better than that of cu
Autor:
A.M. Konovalov, D. G. Rudik, A. Shakirov, G. S. Taer, T. D. Krakhmalova, G. Simakov, Yu.A. Melikyan, A K Berdnikova, A. V. Kumpan, E. Kozlova, A. G. Dolgolenko, D. V. Guss, Yu. V. Gusakov, A. V. Sidorenko, O. E. Nepochataya, Pavel Dzhumaev, V.V. Sosnovtsev, D. Yu. Akimov, M. Yu. Kolpakov, A. G. Kovalenko, V. Belov, A.V. Khromov, A. V. Lukyashin, M. Yu. Savinov, S. V. Bobkov, Alexander Bolozdynya
Publikováno v:
Instruments and Experimental Techniques. 60:782-788
A procedure for spark-discharge purification of a liquid xenon sample with a mass of 55 kg is described. The average lifetime of ionization electrons before capture by electronegative impurities in liquid xenon increased from ≤ 0.1 μs to ≥ 50 μ
Autor:
A. G. Dolgolenko, A.V. Khromov, Yu.A. Melikyan, A. G. Kovalenko, A. A. Tobolkin, Valery V. Dmitrenko, A. Shakirov, V.V. Sosnovtsev, D. G. Rudik, A. M. Konovalov, Yu. Efremenko, P. P. Naumov, E. Kozlova, D. Yu. Akimov, Vladimir Kaplin, Georgy Tikhomirov, A.V. Etenko, A. Burenkov, Yu. V. Gusakov, I. Tolstukhin, Z. M. Uteshev, Alexander Bolozdynya, A. V. Kumpan, Konstantin F. Vlasik, I. S. Aleksandrov, I. S. Saldikov, V. Belov, R. R. Shafigullin, T. D. Krakhmalova
Publikováno v:
Instruments and Experimental Techniques. 60:175-181
The RED-100 experimental setup, which is designed to detect elastic coherent neutrino scattering off xenon nuclei, is described. One specific feature of this setup is the possibility of using it in above ground experiments. The setup is based on the