Geomagnetically trapped antiprotons

Details Geomagnetically trapped antiprotons Geomagnetically trapped antiprotons

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007georl..3420104s&link_type=abstract

Geophysical Research Letters, Volume 34, Issue 20, CiteID L20104

Physics

5

Magnetospheric Physics: Radiation Belts, Magnetospheric Physics: Magnetosphere: Inner, Magnetospheric Physics: Numerical Modeling, Magnetospheric Physics: Energetic Particles: Trapped

Scientific paper

The distribution of geomagnetically trapped antiprotons from decay of cosmic ray albedo antineutrons is described theoretically. The calculation includes ionization energy loss, inelastic nuclear scattering and annihilation, radial diffusion, and solar cycle and geomagnetic secular variations. The trapped antiproton intensity at satellite altitudes is predicted to be significantly higher than the interplanetary cosmic ray antiproton intensity.

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