Interpreting LRO Diviner observations of fine-scale lunar surface thermal variability

Details Interpreting LRO Diviner observations of fine-scale lunar surface thermal variability Interpreting LRO Diviner observations of fine-scale lunar surface thermal variability

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1678w&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1678

Physics

Scientific paper

The Diviner Lunar Radiometer Experiment on NASA's Lunar Reconnaissance Orbiter (LRO) has been mapping the global thermal state of the Moon since July of 2009. The instrument has acquired thermal emission data in nine spectral channels spanning a wavelength range from 0.3 to 400 microns [1]. Surface temperatures are found to exhibit extreme spatial variability. We employ a 3-D regolith heat flow model to aid in interpreting measured brightness temperatures.

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