Annotation
The behavior of various anisotropy parameters as applied to the spatial distribution of cosmic-ray particles in gamma-hadronic families is considered. The sensitivity of the parameters chosen to the type of the parent particle of the given family is established. Using the RUNJOB experimental data, the spatial anisotropy and the alignment effect in cosmic-ray particle interactions at $E_0=10^{13}$-$10^{14}$eV are investigated.
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
V.I. Galkin, A.K. Managadze, V.I. Osedlo, Т.M. Roganova, G. Shoziyoev
Department of Cosmic Rays and Space Physics, Faculty of Physics, Moscow State University, Leninskie Gory, Moscow, 119992, Russia. Institute of Nuclear Physics, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
Department of Cosmic Rays and Space Physics, Faculty of Physics, Moscow State University, Leninskie Gory, Moscow, 119992, Russia. Institute of Nuclear Physics, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
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