Zenith-Angular Characteristics of Particles in EASs with @ eV According to the Yakutsk Array Data
- Authors: Glushkov A.V.1, Lebedev K.G.1, Saburov A.V.1
-
Affiliations:
- Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences
- Issue: Vol 86, No 3 (2023)
- Pages: 379-387
- Section: ЭЛЕМЕНТАРНЫЕ ЧАСТИЦЫ И ПОЛЯ. Эксперимент
- URL: https://journals.rcsi.science/0044-0027/article/view/139735
- DOI: https://doi.org/10.31857/S004400272303011X
- EDN: https://elibrary.ru/RLBPYM
- ID: 139735
Cite item
Abstract
Particle lateral distributions were investigated in cosmic ray air showers with energy
eV registered at the Yakutsk array with surface and underground scintillation detectors with @ GeV threshold during the period of continuous observations from 1986 to 2016. The analysis covers events with arrival direction zenith angles
within five intervals with step
. Experimental values were compared to simulation results obtained with the use of CORSIKA code within the framework of QGSJet-01-d hadron interaction model. The whole dataset points at probable cosmic ray @ omposition which is close to proton one
About the authors
A. V. Glushkov
Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences
Email: glushkov@ikfia.ysn.ru
677027, Yakutsk, Russia
K. G. Lebedev
Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences
Email: vs.tema@gmail.com
677027, Yakutsk, Russia
A. V. Saburov
Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences
Author for correspondence.
Email: vs.tema@gmail.com
677027, Yakutsk, Russia
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