On Primary Cosmic Ray Energy Spectrum Beyond 10 PeV Measured with ENDA-INR

ENDA-INR is a sea level prototype of the running now at high altitude in China ENDA (Electron-Neutron Detector array), being a part of the LHAASO experiment. The main task of the ENDA is measuring of primary cosmic ray energy spectrum using hadronic EAS component. The latter is a principal point because only hadrons form the EAS ‘‘skeleton’’ which defined all its properties at observation level. Preliminary experimental results obtained after 3.7 years of measurements are presented and analyzed.

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Publication Details

Journal
Physics of Atomic Nuclei
Published
2025-12-01
DOI
https://doi.org/10.1134/s1063778825601878
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
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article

On Primary Cosmic Ray Energy Spectrum Beyond 10 PeV Measured with ENDA-INR

I. O. Maliy, V. I. Stepanov, Yu. V. Stenkin, D. A. Kuleshov et al.
Physics of Atomic Nuclei
Astrophysics and Cosmic Phenomena
article

On Primary Cosmic Ray Energy Spectrum Beyond 10 PeV Measured with ENDA-INR

I. O. Maliy, V. I. Stepanov, Yu. V. Stenkin, D. A. Kuleshov, O. B. Shchegolev, K. O. Kurinov
article en

Abstract

ENDA-INR is a sea level prototype of the running now at high altitude in China ENDA (Electron-Neutron Detector array), being a part of the LHAASO experiment. The main task of the ENDA is measuring of primary cosmic ray energy spectrum using hadronic EAS component. The latter is a principal point because only hadrons form the EAS ‘‘skeleton’’ which defined all its properties at observation level. Preliminary experimental results obtained after 3.7 years of measurements are presented and analyzed.

Physics of Atomic NucleiVol. 88(6)
Moscow Institute of Physics and Technology (RU), Moscow Power Engineering Institute (RU), Institute for Nuclear Research (RU)
Life below water
Openalex Percentile: Top 18%
Astrophysics and Cosmic Phenomena
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