Table 1: Hapke parameters of the modeled Mercury image data as a function of wavelength $\lambda $. The initial model is that of Warell (2004) Sol. 1 for the V band. Parameter ranges used while iteratively finding the best solutions are given.
$\lambda $ (nm) w b c h $B_{\rm0}$ $\bar{\theta}$ ($^\circ $)
Initial 0.16 0.18 1.1 0.09 2.7 8
Range 0.1-0.4 0.16-0.20 0.9-1.3 Fixed Fixed 0-40
447 0.14 0.18 1.1 0.09 2.7 20
554 0.18 0.18 1.1 0.09 2.7 20
650 0.22 0.18 1.1 0.09 2.7 20
753 0.26 0.18 1.1 0.09 2.7 20
833 0.28 0.18 1.1 0.09 2.7 20
944 0.32 0.18 1.1 0.09 2.7 20

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