Fig. 10
Our derived rim dust albedos (black circles) calculated using the ratio (0.78 ×IDGL + SBmax)/ISRF and plotted along with the THEMIS model values for the full size distribution of CM, CMM, AMM, and AMMI grains. The grey circles are dust albedos estimated assuming no reduction in DGL (using the ratio (IDGL + SBmax)/ISRF). A reduction of 13% and 7% in albedo values are seen in U and B bands, respectively, with insignificant changes at higher wavelengths for a 22% reduction in DGL intensity.
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