Zobrazeno 1 - 10
of 75
pro vyhledávání: '"Struchkov, G. G."'
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
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
Autor:
Mikhailov, A. A., Efremov, N. N., Gerasimova, N. S., Makarov, I. T., Nikolayeva, G. V., Struchkov, G. G.
It is proposed a new approach for estimating the composition of cosmic rays. It is found that the zenith angle distributions and muon components of EAS for energies E>10^19 eV and E>4.10^19 eV differ from each other. It is shown that the cosmic rays
Externí odkaz:
http://arxiv.org/abs/astro-ph/0507681
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
Autor:
Egorova, V. P., Glushkov, A. V., Ivanov, A. A., Knurenko, S. P., Kolosov, V. A., Krasilnikov, A. D., Makarov, I. T., Mikhailov, A. A., Olzoyev, V. V., Pravdin, M. I., Sabourov, A. V., Sleptsov, I. Ye., Struchkov, G. G
The energy spectrum of primary cosmic rays with ultra high energies based on the Yakutsk EAS Array data is presented. For the largest events values of S600 and axis coordinates have been obtained using revised lateral distribution function. The affec
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411685
Autor:
Knurenko, S. P., Kolosov, V. A., Makarov, I. T., Sleptsov, I. Ye., Sleptsova, V. R., Struchkov, G. G.
Publikováno v:
Int.J.Mod.Phys. A20 (2005) 6900-6902
The ratio of the muon flux density to charged particle flux density at distances of 300 and 600 m from the shower axis ($\rhom(300)/\rhos(300)$ and $\rhom(600)/\rhos(600)$) is measured. In addition, the energy dependence of $\rhom(1000)$ is analysed
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411683
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) 6897-6899
At the Yakutsk EAS array E_em is determined by using measurements of EAS Cherenkov light flux and charged particle flux. It is known from calculations that these characteristics depend on a sort of primary particle and, therefore, the estimation of E
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411682
Autor:
Knurenko, S. P., Egorova, V. P., Ivanov, A. A., Kolosov, V. A., Makarov, I. T., Petrov, Z. E., Sleptsov, I. Ye., Struchkov, G. G.
In the work the data of the Yakutsk complex EAS array and their comparison with calculation in the case of primary nuclei of different chemical elements are presented. The calculation by QGSJET model have been used interpreting experimental data.
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411483
Autor:
Knurenko, S. P., Egorova, V. P., Glushkov, A. V., Ivanov, A. A., Krasilnikov, A. D., Makarov, I. T., Mikhailov, A. A., Olzoyev, V. V., Pravdin, M. I., Sabourov, A. V., Sleptsov, I. Ye., Struchkov, G. G.
Publikováno v:
Int.J.Mod.Phys. A20 (2005) 6878-6881
There are some discrepancies in the results on energy spectrum from Yakutsk, AGASA, and HiRes experiments. In this work differential energy spectrum of primary cosmic rays based on the Yakutsk EAS Array data is presented. For the largest events value
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411484
Autor:
Egorova, V. P., Glushkov, A. V., Ivanov, A. A., Knurenko, S. P., Kolosov, V. A., Krasilnikov, A. D., Makarov, I. T., Mikhailov, A. A., Olzoev, V. V., Pravdin, M. I., Sabourov, A. V., Sleptsov, I. Ye., Struchkov, G. G.
The energy spectrum of UHECRs is discussed on the basis of the Yakutsk array database analysis. In the region E=0.1 to 30 EeV the showers are detected under trigger-500, while at energies above 30 EeV the whole acceptance area for trigger-1000 is use
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408493