Zobrazeno 1 - 10
of 48
pro vyhledávání: '"Sleptsov, I Ye"'
Autor:
Alekseev, A. K., Atlasov, E. A., Bolotnikov, N. G., Bosikov, A. V., Dyachkovskiy, N. A., Gerasimova, N. S., Glushkov, A. V., Ivanov, A. A., Ivanov, O. N., Kardashevsky, D. N., Kellarev, I. A., Knurenko, S. P., Krasilnikov, A. D., Krivenkov, A. N., Ksenofontov, I. V., Ksenofontov, L. T., Lebedev, K. G., Matarkin, S. V., Mokhnachevskaya, V. P., Nikolaeva, E. V., Neustroev, N. I., Petrov, I. S., Platonov, N. D., Proshutinsky, A. S., Sabourov, A. V., Sleptsov, I. Ye., Struchkov, G. G., Timofeev, L. V., Yakovlev, B. B.
Publikováno v:
Physics of Atomic Nuclei 2021 V.84 P.893
The Yakutsk Extensive Air Shower Array has been continuously operating for more than 50 years (since 1970) and up until recently it has been one of world's largest ground-based instruments aimed at studying the properties of cosmic rays in the ultra-
Externí odkaz:
http://arxiv.org/abs/2107.07528
Two EAS arrays during a day have recorded 3 particles with energies above 30 EeV arriving from the same sky region. Two events were registered by the Yakutsk array and one - by the Telescope Array. Two Yakutsk events were estimated to be same energy
Externí odkaz:
http://arxiv.org/abs/1808.08035
Autor:
Ivanov, A. A., Knurenko, S. P., Krasilnikov, A. D., Petrov, Z. E., Pravdin, M. I., Sleptsov, I. Ye., Timofeev, L. V.
Publikováno v:
NIMA, 2015, vol. 772, p. 34
The Yakutsk array group is developing a wide field-of-view Cherenkov telescope to be operated in coincidence with the surface detectors of the extensive air shower array. Currently, the engineering prototype of the reflecting telescope with the front
Externí odkaz:
http://arxiv.org/abs/1404.6595
Autor:
Knurenko, S. P., Petrov, Z. E., Sidorov, R., Sleptsov, I. Ye., Starostin, S. K., Struchkov, G. G.
From the data on Cherenkov light from EASs collected over the period of more than 15 years, the spectrum of cosmic rays was obtained in the energy range 1.0E15-1.0E18 eV. This spectrum has two features: at ~3.0E15 eV (first knee) and at ~1.0E17 eV (s
Externí odkaz:
http://arxiv.org/abs/1310.1978
Publikováno v:
Astrophys. Space Sci. Trans. 6 (2010) 53-57
The aim of the Yakutsk array enhancement project is to create an instrument to study the highest-energy galactic cosmic rays (CRs) -- their sources, energy spectrum, and mass composition. Additionally, there will be unique capabilities for investigat
Externí odkaz:
http://arxiv.org/abs/1011.3902
Publikováno v:
New J.Phys.11:065008,2009
The energy spectrum of cosmic rays in the range 10^15 eV to 6*10^19 eV has been studied using the air Cherenkov light detectors of the Yakutsk array. The total flux of photons produced by relativistic electrons (including positrons as well, hereafter
Externí odkaz:
http://arxiv.org/abs/0902.1016
The characteristics relating to the lateral and longitudinal development of EAS in the energy region of 10^15-10^19eV have been analyzed in the framework of the QGSJET model and of mass composition of primary cosmic rays. It is found that at E(0) >=
Externí odkaz:
http://arxiv.org/abs/0711.2348
The energy dependence of such characteristics as a ratio of the total number of charged particles to the total flux of EAS Cherenkov radiation, a ratio of E(thr)>=1GeV muon flux density at the distance of 600m from a shower core to charged particle f
Externí odkaz:
http://arxiv.org/abs/0711.2130
Publikováno v:
Nucl.Phys.Proc.Suppl.175-176:201-206,2008
Experimental data obtained at the Yakutsk array after the modernization in 1993 are analyzed. The characteristics of EAS longitudinal and radial development found from the charged particle flux and EAS Cherenkov light registered at the Yakutsk comple
Externí odkaz:
http://arxiv.org/abs/astro-ph/0611871
Autor:
Knurenko, S. P., Ivanov, A. A., Kolosov, V. A., Petrov, Z. E., Sleptsov, I. Ye., Struchkov, G. G.
Publikováno v:
Int.J.Mod.Phys. A20 (2005) 6894-6896
The experimental distributions of $\Xmax$ obtained with the Yakutsk EAS array at fixed energies of $5 \times10^{17}$, $1\times10^{18}$ and $5\times10^{18}$ eV are analysed. A recent version of the QGSJET model is used as a tool of our analysis. In th
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411684