Speaker
Dmitry Chernov
(Moscow State University)
Description
The SPHERE-3 setup is destined to register the EAS Cherenkov light, both the direct and the reflected from the snow surface. A set of methods and new approaches in the measurement technique enable substantial progress in the study of the primary cosmic ray composition in the energy range 1-1000 PeV. The present work reveals the current status of the project development and detector performance modeling.
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
