Interpreting LRO Diviner Surface Temperatures: Modeling Lunar Regolith Thermophysical Properties and Topography in Three-Dimensions

Details Interpreting LRO Diviner Surface Temperatures: Modeling Lunar Regolith Thermophysical Properties and Topography in Three-Dimensions Interpreting LRO Diviner Surface Temperatures: Modeling Lunar Regolith Thermophysical Properties and Topography in Three-Dimensions

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2808w&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2808

Physics

Scientific paper

We are developing a three-dimensional finite-difference model of the
lunar regolith including topography and ray tracing to understand how
small-scale slopes, shadows, and rocks within a Diviner surface
footprint influence temperatures derived from Diviner observations.

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