Abstract
An extensive Monte Carlo calculation has been carried out on the propagation of solar flare particles in the energy range 1–100 GeV. The fluxes of neutrons and muons are derived as a function of primary neutron and proton energies. A very interesting result, an inverse muon charge ratio effect, is predicted during solar flare neutron arrivals. This consequence can be applied to high energy neutron emission resulting in the inverse muon charge ratio during bursts of neutron emission by several astronomical objects within a few parsec from Earth.
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