This analysis proposes a method to enhance the accuracy of cosmic ray energy measurement, addressing challenges in cascade development and absorption.
This paper analyzes the problems of determining primary energy using a thin ionization calorimeter. These challenges include large fluctuations in cascade development, a decrease in the statistics of analyzed events with increasing energy, and the need to increase the calorimeter thickness to measure higher-energy particles. To address these challenges, a method is proposed that improves the accuracy of energy determination in direct measurements of cosmic rays with energies of TeV and higher.
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Fedossimova et al. (2025) studied this question.
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