Speaker
Dmitry Chernov
(Moscow State University)
Description
This report presents a draft of a new detector designed to determine the chemical composition of primary cosmic rays based on the characteristics of the angular distribution of Cherenkov light from EAS. The installation, consisting of several such detectors, will be able to register individual EAS events in the energy range from 1 to 1000 PeV with high angular resolution of up to 0.3 degrees. The proposed detector’s distinctive feature is its simple design and wide viewing angle of up to $\pm$30 degrees.
Primary author
Dmitry Chernov
(Moscow State University)
Co-authors
Elena Bonvech
(SINP MSU)
Vladimir Galkin
(Moscow State University, Faculty of Physics & Institute of Nuclear Physics)
Vladimir Ivanov
(Federal State Budget Educational Institution of Higher Education M.V.Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics)
Timofey Kolodkin
(Federal State Budget Educational Institution of Higher Education M.V.Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics)
Natalia Ovcharenko
(Federal State Budget Educational Institution of Higher Education M.V.Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics)
Olga Cherkesova
(SINP MSU)
Dmitriy Podgrudkov
Maxim Ziva
Tatyana Roganova
Elena Entina
