Figure 6From: Cassini/VIMS observes rough surfaces on Titan’s Punga Mare in specular reflectionNear-infrared spectrum. VIMS Near-IR spectrum of three pixels from cube CM_1721848119_1. Two of the bright pixels from the cyan arrows in Figure 2 are shown in red and green, and a nearby reference pixel is in blue. The spectral signature whereby the bright areas are brighter only in the 5 μm window is consistent with their being due to specular reflection.Back to article page