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Interact with the Earth's atmosphere, the cosmic ray protons loss their energy both through the ionization process and through the cascades process. As a result of these interactions, various secondary particles are born. The estimation task of the fluxes for these particles can be applied, for example, in the field of estimating the equivalent dose when flying on airliners at altitudes of 10-11 km. This work presents a method for calculating the secondary particle fluxes formed as a result of the solar cosmic ray protons interaction with the Earth's atmosphere using numerical modeling. To solve this problem, the RUSCOSMICS software package was used, based on the GEANT4 software development tool.