Annotation
The study of the origin and propagation of cosmic rays in the range from 1 to 1000 PeV is important. A new facility, SPHERE-3, with higher luminosity and better optical resolution, is being developed, based on the experience gained from the operation of the balloon facility SPHERE-2. This paper presents a simulation complex for the generation of Cherenkov light images on the detector mosaic of the SPHERE-3 telescope.
Received: 2023 November 15
Approved: 2024 January 17
PACS:
96.50.sb Composition, energy spectra and interactions
96.50.sd Extensive air showers
96.50.sd Extensive air showers
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
V. A. Ivanov, V. I. Galkin
$^1$Moscow State University named after M.V. Lomonosov, physics Faculty, Department of Space Physics
$^1$Moscow State University named after M.V. Lomonosov, physics Faculty, Department of Space Physics
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