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).
@article{arxiv.1704.07681,
title = {A simulation chain for the LAGO Space Weather Program},
author = {Hernan Asorey and Luis A. Núñez and Mauricio Suárez-Durán},
journal= {arXiv preprint arXiv:1704.07681},
year = {2017}
}
Comments
Proceedings XV Latin American Regional IAU Meeting LARIM