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Analysis reveals cosmic ray energy and air shower characteristics, suggesting new insights into cosmic radiation composition.
The results of the operation of the TAIGA-HiSCORE array after increasing the number of stations to 114 and directing all stations to the zenith are presented. The conversion from the measured Cherenkov light flux of the extensive air shower (EAS) to the primary cosmic particle energy is refined. The ⟨ln A⟩ parameter, recalculated from the maximum depth, characterizing the average composition of primary cosmic radiation, is compared with the results obtained at our Tunka-133 installation, as well as with the results of the LHAASO and AUGER experiments.
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V.V. Prosin (2025) studied this question.
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