Tidal Currents Detected in Kraken Mare Straits from Cassini VIMS Sun Glitter Observations
Michael F. Heslar, Jason W. Barnes, Jason M. Soderblom, Benoit, Seignovert, Rajani D. Dhingra, Christophe Sotin

TL;DR
Cassini VIMS sun glitter observations reveal wave activity and tidal currents in Kraken Mare's straits, indicating complex interactions of wind and tidal forces on Titan's liquid surface.
Contribution
First detection of wave activity driven by tidal currents in Kraken Mare using sun glitter observations from Cassini VIMS.
Findings
Wave activity observed in Kraken Mare's straits.
Tidal currents likely influence wave fields in narrow straits.
Wind-driven waves dominate near coastlines, tidal effects in constricted areas.
Abstract
We present Cassini VIMS observations of sun glitter -- wave-induced reflections from a liquid surface offset from a specular point -- on Kraken Mare. Sun glitter reveals rough sea surfaces around Kraken Mare, namely the coasts and narrow straits. The sun glitter observations indicate wave activity driven by the winds and tidal currents in Kraken Mare during northern summer. T104 Cassini VIMS observations show three sun glitter features in Bayta Fretum indicative of variegated wave fields. We cannot uniquely determine one source for the coastal Bayta waves, but we lean toward the interpretation of surface winds, because tidal currents should be too weak to generate capillary-gravity waves in Bayta Fretum. T105 and T110 observations reveal wave fields in the straits of Seldon Fretum, Lulworth Sinus, and Tunu Sinus that likely originate from the constriction of tidal currents. Coastlines…
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