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Fig. 2
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Radial dependence of the fraction of the flux density at 0.8 µm in scattered light due to unbound grains (s < sblοw). Results are shown for the nominal and ‘bright disc’ cases, as well as for anisotropic scattering, at two different angles, using the distribution of hollow spheres model (DHS, Min et al. 2005) for the SPF.
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