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Fig. 33.


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Characteristics of the UHECR dipole for a selected realization. Top: energy evolution of the dipole amplitude predicted for model A, assuming a 1 nG EGMF and the JF12+Planck GMF with λc = 200 pc for a selected realization of the mother catalog sampling for a 10−4 Mpc−3 density (see text). The mean values and the dispersion of the predictions (90% interval) estimated over the 300 datasets are shown respectively with markers and shaded areas and compared to the values reconstructed with Auger data. Bottom: skymaps in galactic coordinates showing the reconstructed directions of the dipoles for each of the 300 datasets in five different energy bins (see the color code legend in Fig. 18). The barycenters of the 300 datasets are shown by large squared markers. The predictions can be compared to the directions reconstructed by Auger shown by full circles and their 1σ error ellipses (large filled circles).

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