Fig. 3.


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Green’s functions of interplanetary transport for λr = 0.5 AU, for two scattering cases: case A (ϵ = 0.01, q = 1.66) and case B (ϵ = 0.10, q = 1.41). From top to bottom: 100–180 keV omni-directional intensity and mean pitch-angle cosine. Normalized pitch-angle distributions are displayed for three snapshots (black dots).

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