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

Мұқаба

Дәйексөз келтіру

Толық мәтін

Ашық рұқсат Ашық рұқсат
Рұқсат жабық Рұқсат берілді
Рұқсат жабық Рұқсат ақылы немесе тек жазылушылар үшін

Аннотация

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.

Авторлар туралы

E. Bonvech

Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University

Email: bonvech@yandex.ru
Moscow, Russia

N. Ovcharenko

Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University; Lomonosov Moscow State University

Moscow, Russia

O. Cherkesova

Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University; Lomonosov Moscow State University

Moscow, Russia

E. Entina

Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University

Moscow, Russia

V. Galkin

Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University; Lomonosov Moscow State University

Moscow, Russia

D. Chernov

Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University

Moscow, Russia

V. Ivanov

Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University; Lomonosov Moscow State University

Moscow, Russia

T. Kolodkin

Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University; Lomonosov Moscow State University

Moscow, Russia

D. Podgrudkov

Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University; Lomonosov Moscow State University

Moscow, Russia

T. Roganova

Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University

Moscow, Russia

M. Ziva

Skobeltsyn Institute for Nuclear Physics, Lomonosov Moscow State University; Lomonosov Moscow State University

Moscow, Russia

Әдебиет тізімі

  1. Чудаков A.E. // Экспериментальные методы исследования космических лучей сверхвысоких энергий. Материалы Всесоюзного симпозиума (Якутск, 1972). С. 69.
  2. Castagnoli C., Navarra G., and Morello C. // Proc. 17th ICRC. 1981. V. 6. P. 103.
  3. Antonov R.A., Ivanenko I.P., and Rubtsov V.I. // Proc. 14th ICRC. 1975. V. 9. P. 3360.
  4. Антонов Р.А., Петрова Е.А., Сысоева Т.И. . и др. // Изв. РАН. Сер. физ. 1999. Т. 63. № 3. С. 520.
  5. Антонов Р.А., Аулова Т.В., Бонвеч Е.А. и др. // ЗНАЯ. 2015. Т. 46. С. 115
  6. Бонвеч Е.А., Чернов Д.В., Латыпова В.С. и др. // Изв. РАН. Сер. физ. 2024. Т. 88. № 3. С. 518
  7. Heck D., Knapp J., Capdevielle J.N. et al. // FZKA-6019. Karlsruhe: Forschungszentrum Karlsruhe, 1998.
  8. Chernov D.V., Kolodkin T.A., Ivanov V.A. et al. // Bull. Russ. Acad. Sci. Phys. 2025. V. 89. No. 6. P. 1002.
  9. Voevodin V.V., Antonov A.S., Nikitenko D.A. et al. // Supercomp. Front. Innovations. 2019. V. 6. No. 2. P. 4.
  10. Agostinelli S., Allison J., Amako K. et al. // Nucl. Instrum. Meth. A. 2003. V. 506. P. 250.

Қосымша файлдар

Қосымша файлдар
Әрекет
1. JATS XML
Жүктеу

© Russian Academy of Sciences, 2025