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Fig. 7

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Differential flux of dust collected in each mass bin normalized to the solar distance at 3 AU and to 10 km distance from the comet assuming . The conversion from size to mass is done assuming a constant density of 1000 kg/m3 (black dots) and a size-dependant density (open circles) with ρ0 = 1 g/cm3 for r0 = 1 μm. The vertical error bars take into account the different confidence limits; as in Fig. 3a, the horizontal error bars represent the sizes of the mass bins. The size reported on the top x axis is derived using a density of 1000 kg/m3.

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