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Orbital detector of ultra-high-energy cosmic rays: status and prospects of the KLYPVE project
- Authors: Belov A.A.1,2, Klimov P.A.1, Sharakin S.A.1, Zotov M.Y.1
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Affiliations:
- Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
- Lomonosov Moscow State University, Faculty of Physics
- Issue: Vol 87, No 7 (2023)
- Pages: 923-926
- Section: Articles
- URL: https://innoscience.ru/0367-6765/article/view/654339
- DOI: https://doi.org/10.31857/S0367676523701600
- EDN: https://elibrary.ru/ONCCMD
- ID: 654339
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Abstract
KLYPVE (K-EUSO) is a planned space experiment aimed at studying ultra-high-energy cosmic rays by detecting fluorescent and Cherenkov radiation from extensive air showers in the Earth’s night atmosphere from near-Earth orbit. The observatory is being developed as a part of the JEM-EUSO program. The registration threshold will be about 50 EeV, and the annual statistics of events will be more than 50. The KLYPVE mission can significantly supplement the data of ground-based experiments.
About the authors
A. A. Belov
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics; Lomonosov Moscow State University, Faculty of Physics
Email: pavel.klimov@gmail.com
Russia, 119991, Moscow; Russia, 119991, Moscow
P. A. Klimov
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Author for correspondence.
Email: pavel.klimov@gmail.com
Russia, 119991, Moscow
S. A. Sharakin
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Email: pavel.klimov@gmail.com
Russia, 119991, Moscow
M. Yu. Zotov
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Email: pavel.klimov@gmail.com
Russia, 119991, Moscow
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