Estimates of Galactic Cosmic Ray Spectra at Low Energies

Computer Science

Scientific paper

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Scientific paper

A simple model including shock acceleration, energy loss, and
propagation loss is employed to calculate the energy spectra of cosmic
ray protons, alpha particles, and electrons between 1 MeV/nuc and 100
GeV/nuc. On the basis of these theoretical results, the energy density
and pressure density of the cosmic ray particles are also computed.

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