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Cassini/VIMS high-phase specular observations of Titan's north pole during the T85 flyby show evidence for isolated patches of rough liquid surface within the boundaries of the sea Punga Mare. The roughness shows typical slopes of 6° ± 1°. These rough areas could be either wet mudflats or a wavy sea. Because of their large areal extent, patchy geographic(More)
Throughout the course of my Ph.D. program, I have worked on a multitude of different projects, many of which do not appear in this thesis. Nonetheless, I'd like to acknowledge here everyone who has made a significant contribution to my research and education in the past several years. First, I would like to acknowledge my research advisor, Chris Ruf. I, as(More)
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