Status of the K-EUSO Orbital Detector of Ultra-High Energy Cosmic Rays

被引：17

作者：

Klimov, Pavel ^{[1
]}

Battisti, Matteo ^{[2
]}

Belov, Alexander ^{[1
,3
]}

Bertaina, Mario ^{[2
]}

Bianciotto, Marta ^{[2
]}

Blin-Bondil, Sylvie ^{[4
,5
]}

Casolino, Marco ^{[6
]}

Ebisuzaki, Toshikazu ^{[6
]}

Fenu, Francesco ^{[2
]}

Fuglesang, Christer ^{[8
]}

Marszal, Wlodzimierz ^{[9
]}

Neronov, Andrii ^{[4
,10
]}

Parizot, Etienne ^{[4
]}

Picozza, Piergiorgio ^{[6
,7
,11
]}

Plebaniak, Zbigniew ^{[2
]}

Prevot, Guillaume ^{[4
]}

Przybylak, Marika ^{[9
]}

Sakaki, Naoto

Sharakin, Sergey ^{[1
]}

Shinozaki, Kenji ^{[9
]}

Szabelski, Jacek ^{[9
]}

Takizawa, Yoshiyuki ^{[6
]}

Trofimov, Daniil ^{[1
]}

Yashin, Ivan ^{[1
]}

Zotov, Mikhail ^{[1
]}

机构：

[1] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow 119991, Russia

[2] Univ Torino, Dept Phys, Via Pietro Giuria 1, I-10125 Turin, Italy

[3] Moscow MV Lomonosov State Univ, Fac Phys, Moscow 119991, Russia

[4] Univ Paris, CNRS, Astroparticule & Cosmol, F-75013 Paris, France

[5] CNRS, Ecole Polytechn, IN2P3, Omega, F-91128 Palaiseau, France

[6] RIKEN, Wako, Saitama 3510198, Japan

[7] INFN, Struct Rome Tor Vergata, I-00133 Rome, Italy

[8] KTH Royal Inst Technol, SE-10044 Stockholm, Sweden

[9] Natl Ctr Nucl Res, PL-90558 Lodz, Poland

[10] Ecole Polytechn Federale Lausanne, Lab Astrophys, CH-1015 Lausanne, Switzerland

[11] Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy

来源：

UNIVERSE | 2022年 / 8卷 / 02期

关键词：

ultra-high energy cosmic rays; fluorescence telescope; orbital experiment; K-EUSO; JEM-EUSO; NEURAL-NETWORKS; TUS; KLYPVE;

D O I：

10.3390/universe8020088

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

K-EUSO (KLYPVE-EUSO) is a planned orbital mission aimed at studying ultra-high energy cosmic rays (UHECRs) by detecting fluorescence and Cherenkov light emitted by extensive air showers in the nocturnal atmosphere of Earth in the ultraviolet (UV) range. The observatory is being developed within the JEM-EUSO collaboration and is planned to be deployed on the International Space Station after 2025 and operated for at least two years. The telescope, consisting of & SIM;10(5 )independent pixels, will allow a spatial resolution of & SIM;0.6 km on the ground, and, from a 400 km altitude, it will achieve a large and full sky exposure to sample the highest energy range of the UHECR spectrum. We provide a comprehensive review of the current status of the development of the K-EUSO experiment, paying special attention to its hardware parts and expected performance. We demonstrate how results of the K-EUSO mission can complement the achievements of the existing ground-based experiments and push forward the intriguing studies of ultra-high energy cosmic rays, as well as bring new knowledge about other phenomena manifesting themselves in the atmosphere in the UV range.

引用

页数：22

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