Spatiotemporal Structure of a Reflected Cherenkov Light Signal, as Seen by the Sphere-2 Telescope


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Resumo

SPHERE-2 is a Cherenkov telescope suspended under a tethered balloon and observing the optical Vavilov–Cherenkov radiation of extensive air showers (EAS) reflected from the snowy surface of Lake Baikal. Extended modeling of the SPHERE-2 detector’s response is done with a specially developed code. Resulting model events resemble EASes observed during observation runs at Lake Baikal. This work should facilitate event-by-event studies of cosmic ray mass composition in the 10–100 PeV range of energies.

Sobre autores

E. Bonvech

Skobeltsyn Institute of Nuclear Physics, Moscow State University

Autor responsável pela correspondência
Email: chr@sinp.msu.ru
Rússia, Moscow, 119991

V. Galkin

Faculty of Physics, Moscow State University

Email: chr@sinp.msu.ru
Rússia, Moscow, 119991

T. Dzhatdoev

Skobeltsyn Institute of Nuclear Physics, Moscow State University

Email: chr@sinp.msu.ru
Rússia, Moscow, 119991

D. Podgrudkov

Faculty of Physics, Moscow State University

Email: chr@sinp.msu.ru
Rússia, Moscow, 119991

T. Roganova

Skobeltsyn Institute of Nuclear Physics, Moscow State University

Email: chr@sinp.msu.ru
Rússia, Moscow, 119991

D. Chernov

Faculty of Physics, Moscow State University

Email: chr@sinp.msu.ru
Rússia, Moscow, 119991

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