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The Isotropy Problem of Sub-ankle Ultra High Energy Cosmic Rays
Kumar & Eichler 2014 The Astrophysical Journal 781 47.
Caption: Figure 4.
Temporal variation of anisotropy and flux as in Figure 3, but for λ mfp = 3 r L . All other details are same as in Figure 3.
© 2014. The American Astronomical Society. All rights reserved.
