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Fig. 6

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The lunar mare volume-element phase function of Fig. 5 averaged using bin size of 0.5°. We show the best-fit volume-element scattering phase function PV (solid line). For the largest phase angles, there is a deviation that is probably due to the incapability of the present model volume-element phase function to fit the observations and to increasing real brightness variegation or correlated observational errors.

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