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16.1} Primary spectrum

 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).
 Two options are available: with the first one the actual ion composition
 of the flux is used (All-Particle Spectrum), while with the second option
 the primary flux is treated as a sum of nucleons (All-Nucleon Spectrum).

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