The primary cosmic-ray energy spectrum measured with the Tunka-133 array
High Energy Astrophysical Phenomena
2021-04-09 v1
Abstract
The EAS Cherenkov light array Tunka-133, with 3 km geometric area, is taking data since 2009.The array permits a detailed study of energy spectrum and mass composition of cosmic rays in the energy range from to eV. We describe the methods of time and amplitude calibration of the array and the methods of EAS parameters reconstruction. We present the all-particle energy spectrum, based on 7 seasons of operation.
Cite
@article{arxiv.2104.03599,
title = {The primary cosmic-ray energy spectrum measured with the Tunka-133 array},
author = {N. M. Budnev and A. Chiavassa and O. A. Gress and T. I. Gress and A. N. Dyachok and N. I. Karpov and N. N. Kalmykov and E. E. Korosteleva and V. A. Kozhin and L. A. Kuzmichev and B. K. Lubsandorzhiev and N. B. Lubsandorzhiev and R. R. Mirgazov and E. A. Osipova and M. I. Panasyuk and L. V. Pankov and E. G. Popova and V. V. Prosin and V. S. Ptuskin and Yu. A. Semeney and A. A. Silaev and A. A. Silaev and A. V. Skurikhin and C. Spiering and L. G. Sveshnikova},
journal= {arXiv preprint arXiv:2104.03599},
year = {2021}
}
Comments
12 pages,18 figures