P o S ( I C R C 2 0 1 5 ) 1 8 3 Cosmic Rays Propagation with HelMod : Difference between forward-intime and backward-intime approaches
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S. Pensotti | P. Rancoita | M. Zannoni | M. Gervasi | M. Putiš | D. Rozza | S. D. Torre | P. Bobik | M. Boschini | D. Grandi | M. Tacconi | G. Vacca