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


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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.

作者简介

E. Bonvech

Skobeltsyn Institute of Nuclear Physics, Moscow State University

编辑信件的主要联系方式.
Email: chr@sinp.msu.ru
俄罗斯联邦, Moscow, 119991

V. Galkin

Faculty of Physics, Moscow State University

Email: chr@sinp.msu.ru
俄罗斯联邦, Moscow, 119991

T. Dzhatdoev

Skobeltsyn Institute of Nuclear Physics, Moscow State University

Email: chr@sinp.msu.ru
俄罗斯联邦, Moscow, 119991

D. Podgrudkov

Faculty of Physics, Moscow State University

Email: chr@sinp.msu.ru
俄罗斯联邦, Moscow, 119991

T. Roganova

Skobeltsyn Institute of Nuclear Physics, Moscow State University

Email: chr@sinp.msu.ru
俄罗斯联邦, Moscow, 119991

D. Chernov

Faculty of Physics, Moscow State University

Email: chr@sinp.msu.ru
俄罗斯联邦, Moscow, 119991

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