Figure 1
From: Cassini/VIMS observes rough surfaces on Titan’s Punga Mare in specular reflection
Cube CM_1721848119_1. Cassini Visual and Infrared Mapping Spectrometer (VIMS) cube CM_1721848119_1 from the T85 Titan flyby on 2012 July 24. This cube shows a bright specular reflection (sunglint) off Kivu Lacus. This interpolated color version uses 2.0 μm as blue, 2.8 μm as green, and 5.0 μm as red. The complex structure surrounding the central glint is described in Barnes et al. ([20]).