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Fig. 1


All-sky maps of simulated ribbon flux, centered on the LISM inflow direction (i.e., Nose). We show results for the uniform slow (left column), intermediate (middle column), and fast (right column) SW, for IBEX-Hi energy passbands 2–6 (top-down). The directions toward the nose, Voyager 1 (V1), and Voyager 2 (V2) are shown. Note the color bar scales are the same for each SW case, but different for each energy. The color scales are the same as those used in Fig. 2 of Schwadron et al. (2014).

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