Modeled water production rate as a function of heliocentric distance from 4 AU inbounds in comparison with measurements. Measurements are marked by discrete symbols. MIRO data are given by Gulkis et al. (2015). All other data are adapted from Fig. 15 in Fougere et al. (2016). Model results assuming different thickness of the overlying dust mantle for f= 0.1 are indicated by solid blue lines. The solid red curve corresponds to f= 0.01 with a mantle thickness of 5 mm.
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