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The Isotropy Problem of Sub-ankle Ultra High Energy Cosmic Rays

  • Authors: Rahul Kumar and David Eichler

Kumar & Eichler 2014 The Astrophysical Journal 781 47.

  • Provider: AAS Journals

Caption: Figure 3.

Top panel: 5 Myr light curve of the local proton flux in arbitrary units for two different source rates: the dotted (blue) curve is for source rate 10 −2 yr −1, and the solid (green) curve is for 10 −4 yr −1. Bottom panel: Temporal variation of the anisotropy is plotted for two different source rates as in the top panel. The dashed (red) line indicates the 99% upper limit set by Auger. Here the GMF is chosen to be MF1 and λ mfp = r L .

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