The Dunes of Shangri-La : New Cassini RADAR results on patterns of aeolian features and the influence of topography

Details The Dunes of Shangri-La : New Cassini RADAR results on patterns of aeolian features and the influence of topography The Dunes of Shangri-La : New Cassini RADAR results on patterns of aeolian features and the influence of topography

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufm.p21a1309l&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #P21A-1309

Physics

3307 Boundary Layer Processes, 3319 General Circulation (1223), 3346 Planetary Meteorology (5445, 5739), 5470 Surface Materials And Properties, 6281 Titan

Scientific paper

Recent flybys (T43, T44 - and just prior to this meeting, T48) provide SAR imagery of northern Shangri-La, the large dark region just to the WNW of Xanadu. Previous imaging of SE Shangri-La (T13) showed that dunes there take a pronounced southward dip compared with the E-W direction seen elsewhere. The new data show rather different directions for dunes in northern Shangri-La, and confirm a blocking or divergent influence of Xanadu. Application of monopulse radar methods to retrieve elevations from Cassini SAR images ('SARTopo') now allows us to explore the influence of topography on the local dune (and by implication, wind) patterns, and the relationship between elevation and sediment accumulation. The lack of large positive relief at Xanadu makes its influence on the dunes somewhat surprising. We consider the possible mechanisms of Xanadu's effect on the winds, using terrestrial analogs as a guide. We review the global pattern of dune orientations and their implications for atmospheric circulation: this orientation map presents a challenging constraint for modelers. We note preliminary indications that scatterometry of Titan's dunefields yields azimuth-dependent radar cross-sections (as is the case for terrestrial sand seas) and note future plans for dune studies on Titan with multi-angle observations that will provide constraints on dune-scale slopes and duneforms too small to resolve.

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