Figure 2From: Cassini/VIMS observes rough surfaces on Titan’s Punga Mare in specular reflection5- μm image. Here we show the 5- μm window of cube CM_1721848119_1, scaled from I/F=0.0 to I/F=0.44. Red indicates the saturation of pixels, which occurs at the primary specular reflection off Kivu Lacus. The arrows indicate the areas of interest for this paper, which show specular reflections on Punga Mare away from the specular point that may represent wave activity.Back to article page