Figure 11From: Cassini/VIMS observes rough surfaces on Titan’s Punga Mare in specular reflectionWave fit. Plot of the specular flux from 4 points on Punga Mare at 5 μm from cube CM_1721848119_1 (asterisks) as a function of the specular facet deviation θ, along with a line representing the result of a χ2 minimization fit with σ=5.8°.Back to article page