Angular power spectra of ultra-high energy cosmic rays traveling through the galactic magnetic field

Details Angular power spectra of ultra-high energy cosmic rays traveling through the galactic magnetic field Angular power spectra of ultra-high energy cosmic rays traveling through the galactic magnetic field

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aph....29...87m&link_type=abstract

Astroparticle Physics, Volume 29, Issue 2, p. 87-93.

Other

Cosmic-Ray Interactions, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays

Scientific paper

We use the method of calculating spherical harmonics coefficients to model the behavior of ultra-high energy cosmic rays through the galactic magnetic field (GMF). By tracking antiprotons out to a certain distance, then using their positions on the sky to determine the probability of UHECR coming from that direction before reinjecting them toward a detector, we can realistically simulate the effect the GMF would have on incoming UHECR particles’ observed distributions at the Earth’s surface.

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