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Specular Reflections from Titan’s Punga Mare Seen by Cassini/VIMS Indicate Surface Roughness: Waves?. Jason W. Barnes Associate Professor of Physics University of Idaho and the Cassini VIMS Team. Lunar and Planetary Science Conference 2014 March 17 Houston, TX. T85 CM_1721848119_1.
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Specular Reflections from Titan’s Punga Mare Seen by Cassini/VIMS Indicate Surface Roughness: Waves? Jason W. Barnes Associate Professor of Physics University of Idaho and the Cassini VIMS Team Lunar and Planetary Science Conference 2014 March 17 Houston, TX
Bottomless Lakes, NM (thanks Karl Mitchell)
Conclusions • Off-specular signal in Punga Mare from T85 indicates roughened, liquid surface • Typical slope angle 6 +/- 1 degrees • Possibilities: • Waves • Wet, liquid-covered mudflat • Moist or partially dry surface • Waves seems most likely, given T94 VIMS obs of Punga, and spatially isolated nature of wave activity • Isolated wave patches, locally induced by winds just at or above threshold – 2cm high • First extraterrestrial ocean waves! • Titan’s seas are liquid, and don’t have viscosity of molasses • Indicates winds picking up as northern spring progresses? • Specular wave searches can constrain winds in the future