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Fig. 11


Summary of fit between observational datasets and the model for COBE data (a) and the lunar microcrater number distribution (b), and meteor data for the helion (c), apex (d), and toroidal (e) categories. Finally, a comparison is shown between the cumulative flux (spinning plate) at Earth for this model and from Grün et al. (1985) (f). Population weighting 80% JFC, 0.5% HTC, and 19.5% JFC. Fcoll = [1 1 1 1 1 1 50 50 50 50 50 50]. Mass distribution α = 5, β = 2, Dmid = 150 μm.

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