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Deflection of ultra high energy cosmic rays by the galactic magnetic field: from the sources to the detector

The Astrophysical Journal, no. 1 (1998): 200-204

Cited by: 77|Views14

Abstract

We report the results of 3D simulations of the trajectories of ultra-high energy protons and Fe nuclei (with energies $E = 4 \times 10^{19}$ and $2.5 \times 10^{20} eV$) propagating through the galactic magnetic field from the sources to the detector. A uniform distribution of anti-particles is backtracked from the detector, at the Earth,...More

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