Measurements of Cosmic Proton Flux through Neutron Monitors Using Deep Networks and Imputation Techniques in the AMS-02 Era

Abstract Accurate measurements of cosmic proton flux are essential for studying the modulation processes of cosmic rays during the solar activity cycle. A proton flux measurement method, based on ground-based neutron monitor (NM) data and deep learning techniques, is presented. After the necessary preprocessing of ground-based NM data using a convolutional neural network model, we model the relationship between NM observations and proton flux measured by the Alpha Magnetic Spectrometer (AMS). The daily cosmic proton flux, ranging from 1 to 100 GV, is obtained for the period from 2011 to 2024 and shows strong agreement with the observed values. In addition, daily proton flux is computed for periods when AMS measurements were unavailable for operational reasons. For the first time, hourly proton flux as a function of rigidity is calculated for the study of short-time solar activity.