A simulation chain for the LAGO Space Weather Program

Published 25 Apr 2017 in physics.space-ph and astro-ph.IM | (1704.07681v1)

Abstract: We simulate the expected variations of background flux at two particular sites of the Latin American Giant Observatory (LAGO) and found that these fluxes are sensible to the latitude and that neutrons and muons components, of cosmic rays, are affected due to the variation of the geomagnetic field (GF).

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