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The Ultra-High-Energy Cosmic Ray Fluorescent Detector of the EUSO-SPB2 Project

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Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

The authors describe a EUSO-SPB2 balloon experiment to study ultra-high energy and extreme energy cosmic rays along with high-energy astrophysical neutrinos. The main characteristics of the fluorescent and Cherenkov telescopes are given. A multi-channel photodetectoris calibrated as part of the pre-flight preparation.

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Funding

This work was supported by ongoing institutional funding. No additional grants to carry out or direct this particular research were obtained.

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Authors and Affiliations

  1. Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119991, Moscow, Russia

    A. A. Belov, P. A. Klimov & D. A. Trofimov

  2. Moscow State University, 119991, Moscow, Russia

    A. A. Belov & D. A. Trofimov

  3. Université Paris Cité, CNRS, Astroparticule et Cosmologie, 75013, Paris, France

    D. A. Trofimov

Authors
  1. A. A. Belov
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  2. P. A. Klimov
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  3. D. A. Trofimov
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Corresponding author

Correspondence to D. A. Trofimov.

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The authors of this work declare that they have no conflicts of interest.

Additional information

Translated by V. Polyakov

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Belov, A.A., Klimov, P.A. & Trofimov, D.A. The Ultra-High-Energy Cosmic Ray Fluorescent Detector of the EUSO-SPB2 Project. Bull. Russ. Acad. Sci. Phys. 88, 424–426 (2024). https://doi.org/10.1134/S1062873823705640

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  • DOI: https://doi.org/10.1134/S1062873823705640

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