电邮这篇文章 Orbital detector of ultra-high-energy cosmic rays: status and prospects of the KLYPVE project
- 作者: Belov A.A.1,2, Klimov P.A.1, Sharakin S.A.1, Zotov M.Y.1
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隶属关系:
- Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
- Lomonosov Moscow State University, Faculty of Physics
- 期: 卷 87, 编号 7 (2023)
- 页面: 923-926
- 栏目: Articles
- URL: https://edgccjournal.org/0367-6765/article/view/654339
- DOI: https://doi.org/10.31857/S0367676523701600
- EDN: https://elibrary.ru/ONCCMD
- ID: 654339
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详细
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.
作者简介
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. Klimov
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
编辑信件的主要联系方式.
Email: pavel.klimov@gmail.com
Russia, 119991, Moscow
S. Sharakin
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Email: pavel.klimov@gmail.com
Russia, 119991, Moscow
M. Zotov
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Email: pavel.klimov@gmail.com
Russia, 119991, Moscow
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