Estimation of extensive air shower primary parameters using angular distribution of the Cherenkov light in the SPHERE-3 experiment

E. A Bonvech; Бонвеч Е. А; N. O Ovcharenko; Овчаренко Н. О; O. V Cherkesova; Черкесова О. В; E. L Entina; Энтина Е. Л; V. I Galkin; Галкин В. И; D. V Chernov; Чернов Д. В; V. A Ivanov; Иванов В. А; T. A Kolodkin; Колодкин Т. А; D. A Podgrudkov; Подгрудков Д. А; T. M Roganova; Роганова Т. М; M. D Ziva; Зива М. Д

doi:10.31857/S0367676525060317

Estimation of extensive air shower primary parameters using angular distribution of the Cherenkov light in the SPHERE-3 experiment

作者: Bonvech E.A¹, Ovcharenko N.O¹^,2, Cherkesova O.V¹^,2, Entina E.L¹, Galkin V.I¹^,2, Chernov D.V¹, Ivanov V.A¹^,2, Kolodkin T.A¹^,2, Podgrudkov D.A¹^,2, Roganova T.M¹, Ziva M.D¹^,2
隶属关系:
1. Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University
2. Lomonosov Moscow State University
期: 卷 89, 编号 6 (2025)
页面: 994-998
栏目: Physics of Cosmic Rays
URL: https://journals.rcsi.science/0367-6765/article/view/321459
DOI: https://doi.org/10.31857/S0367676525060317
ID: 321459

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Some plans for the development of the SPHERE experiment are presented. Namely, reasons for the introduction of an additional detector of the angular distribution of Cherenkov light, pointed at zenith, are given. It can only work together with the main telescope but can yield important information on the primary particle direction and mass. Construction and capabilities of the detector are discussed, draft algorithms for direction definition are revealed, and sensitivity to the primary mass is shown.

关键词

extensive air shower, Cherenkov light, Monte Carlo simulation, primary cosmic rays

参考

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卷 89, 编号 6 (2025)

Estimation of extensive air shower primary parameters using angular distribution of the Cherenkov light in the SPHERE-3 experiment

全文:

详细

关键词

作者简介

E. Bonvech

N. Ovcharenko

O. Cherkesova

E. Entina

V. Galkin

D. Chernov

V. Ivanov

T. Kolodkin

D. Podgrudkov

T. Roganova

M. Ziva

参考

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