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Primary GCR interact with the Earth's atmosphere originating atmosphericshowers, thus giving rise to fluxes of secondary particles in the atmosphere.Electromagnetic and hadronic interactions interplay in the production of theseparticles, whose detection is performed by means of complementary techniques indifferent energy ranges and at different depths in the atmosphere, down to theEarth's surface.  Monte Carlo codes are essential calculation tools which can describe thecomplexity of the physics of these phenomena, thus allowing the analysis ofexperimental data. However, these codes are affected by importantuncertainties, concerning, in particular, hadronic physics at high energy. Inthis paper we shall report some results concerning inclusive particle fluxesand atmospheric shower properties as obtained using the FLUKA transport andinteraction code. Some emphasis will also be given to the validation of thephysics models of FLUKA involved in these calculations.

Secondary Cosmic Ray particles due to GCR interactions in the Earth's atmosphere