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Figure 8
Calculated scattering from ensembles of spheres with number density varying as a function of radius, N(r) = ra. The heterogeneous distribution of radii fills in the troughs in the calculated scattering from a single sphere (seen in Fig. 6[link]). It also mixes scattering patterns that have different qmin below which the power-law behavior ends. That leads to scattering with different apparent slopes. Left: scattering from ten ensembles with a = [1,10]. Right: linear fits to the calculated intensities for a = [1,4].

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