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Fig. E.1


Disk-integrated phase curves for FI and FQ/FI for a Rayleigh-scattering atmosphere with ϖ = 1 and rg = 1 and optical thicknesses from 0.1 to 10. Our PBMC calculations for nph = 104 (red curves) are compared to the calculations by Buenzli & Schmid (2009) using a forward Monte Carlo algorithm (black curves) and at least 2 × 106 photons per exit direction bin over the 30–120°α-range. Both sets of curves are nearly indistinguishable on the scale of the graph, even for the relatively small number of photon realisations used in our PBMC calculations.

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