Origin of the high energy proton component below the geomagnetic cutoff in near earth orbit

Details Origin of the high energy proton component below the geomagnetic cutoff in near earth orbit Origin of the high energy proton component below the geomagnetic cutoff in near earth orbit

2000-06-12

arxiv.org/abs/astro-ph/0006160v2

Phys.Lett. B489 (2000) 1-8

Astronomy and Astrophysics

Astrophysics

7 pages, Latex, 4 Postscript figures. Final version (minor corrections) for Physics Letters. B

Scientific paper

10.1016/S0370-2693(00)00914-X

The high flux proton component observed by AMS below the geomagnetic cutoff
can be well accounted for by assuming these particles to be secondaries
originating from the interaction of Cosmic Ray protons with the atmosphere.
Simulation results are reported

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