24-26 June 2025
National Research Nuclear University MEPhI
Europe/Moscow timezone

Estimation of the capabilities of the SPHERE-3 Cherenkov telescope by determining the parameters of the primary cosmic particles.

Not scheduled
15m
National Research Nuclear University MEPhI

National Research Nuclear University MEPhI

Kashirskoe shosse 31, Moscow, Russian Federation, 115409
Original Talk Cosmic rays (nuclei, gammas, neutrinos) of very high energies (> 100 TeV) Cosmic rays (nuclei, gammas, neutrinos) of very high energies (> 100 TeV)

Speaker

Elena Bonvech (SINP MSU)

Description

New results of modelling the operation of the new Cherenkov telescope SPHERE-3 are presented. The telescope will be able to detect cosmic particles by direct and reflected Cherenkov light of EAS. Dual detection improves the accuracy of determining the parameters of the primary particle. The study is based on the data bank of distributions of the EAS Cherenkov light obtained on the Lomonosov-2 supercomputer. The accuracy of determining the energy and type of the primary particle from the reflected and direct flux of Cherenkov light is estimated.

Primary author

Elena Bonvech (SINP MSU)

Co-authors

Vladimir Galkin (Moscow State University, Faculty of Physics & Institute of Nuclear Physics) Olga Cherkesova (SINP MSU) Timofey Kolodkin (Federal State Budget Educational Institution of Higher Education M.V.Lomonosov Moscow State University, Skobeltsyn 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) Elena Entina Tatyana Roganova Dmitriy Podgrudkov Natalia Ovcharenko (Federal State Budget Educational Institution of Higher Education M.V.Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics) Maxim Ziva Dmitry Chernov (Moscow State University)

Presentation Materials

There are no materials yet.