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Energy spectrum and mass composition of cosmic rays, by the data of the Tunka-133 array

  • Materials of the XXXIII National Conference on Cosmic Rays
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Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

The Tunka-133 Cherenkov light array for the detection of extensive air showers (EAS) acquires data over the five winters from 2009 to 2014. The direction of arrival, the shower core coordinates on the plane of observation, the primary energy, and the depth of the shower maximum are reconstructed for each EAS. A differential all-particle energy spectrum is obtained in the energy range of 6 × 1015–3 × 1018 eV over 1540 h, along with the energy dependence of the average depth of the shower maximum in the range of 6 × 1016–3 × 1018 eV. Based on this dependence, the variation in the average composition of the primary cosmic rays is estimated as a function of energy.

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Correspondence to V. V. Prosin.

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Original Russian Text © S.F. Berezhnev, N.M. Budnev, O.A. Gress, A.N. Dyachok, S.N. Epimakhov, A.V. Zagorodnikov, N.N. Kalmykov, N.I. Karpov, V.A. Kozhin, E.N. Konstantinov, A.V. Korobchenko, E.E. Korosteleva, L.A. Kuzmichev, A. Chiavassa, B.K. Lubsandorzhiev, N.B. Lubsandorzhiev, R.R. Mirgazov, R.D. Monkhoev, E.A. Osipova, M.I. Panasyuk, L.V. Pankov, A.L. Pakhorukov, E.G. Popova, V.V. Prosin, V.S. Ptuskin, L.G. Sveshnikova, Yu.A. Semeney, A.A. Silaev (Sr), A.A. Silaev (Jr), A.V. Skurikhin, O.A. Chvalaev, C. Spiering, I.V. Yashin, 2015, published in Izvestiya Rossiiskoi Akademii Nauk. Seriya Fizicheskaya, 2015, Vol. 79, No. 3, pp. 377–380.

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Berezhnev, S.F., Budnev, N.M., Gress, O.A. et al. Energy spectrum and mass composition of cosmic rays, by the data of the Tunka-133 array. Bull. Russ. Acad. Sci. Phys. 79, 344–347 (2015). https://doi.org/10.3103/S1062873815030090

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  • DOI: https://doi.org/10.3103/S1062873815030090

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