A. V. Glushkov, L. T. Ksenofontov, K. G. Lebedev, A. V. Saburov
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引用次数: 0
Abstract
In this article a new method is proposed for estimating the mass composition of cosmic rays in individual events with energies above \(1.25 \times {{10}^{{19}}}\) eV. It is based on a joint analysis of experimental data and simulation results obtained using the QGSjet-II.04 model for muons with threshold energy \({{E}_{\mu }} = 1.0 \times \cos \theta \) GeV in air showers with zenith angles up to 60°. The data from ground-based and underground scintillation detectors of the Yakutsk EAS array were used. Separate groups of nuclei and other primary particles were found.
期刊介绍:
All topics of experimental and theoretical physics including gravitation, field theory, elementary particles and nuclei, plasma, nonlinear phenomena, condensed matter, superconductivity, superfluidity, lasers, and surfaces.