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The Galactic Cosmic Ray (GCR) component of the cosmic ray flux can be simulated up to 30 TeV/nucleon (or 500 TeV/n when DPMJET is linked). Three options are available: with the first two the actual ion composition of the flux is used (AMS All-Particle Spectrum, Old All-Particle Spectrum), while with the thrid option the primary flux is treated as a sum of nucleons (All-Nucleon Spectrum).