Relative Flux Across the Sky in Backtracked UHECR Simulations

Details Relative Flux Across the Sky in Backtracked UHECR Simulations Relative Flux Across the Sky in Backtracked UHECR Simulations

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010head...11.3207b&link_type=abstract

American Astronomical Society, HEAD meeting #11, #32.07; Bulletin of the American Astronomical Society, Vol. 41, p.704

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Simulation of Ultra High Energy Cosmic Rays traversal of the Galactic Magnetic Field from extra-galactic sources can be extremely computationally intensive. As such many backtrack particle from Earth through the GMF model being tested. Presented here is a method for accounted for relative flux variations across the sky due to magnetic focusing.

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