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Fig. 7


Simulated particle flux compared with in-situ measurements by New Horizons and Voyager 1 and 2. The solid black line takes into account planets and sublimation and represents our best fit to the data taken from Poppe et al. (2010), Han et al. (2011) and Gurnett et al. (1997). The dotted and dashed lines show the dust flux for the unperturbed EKB and after planetary scattering without sublimation, respectively.

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