Spectral Thermal Emission of the Lunar Surface: Implications for Mapping of the Surficial Volatiles and Monitoring Variations with Time of Day

Details Spectral Thermal Emission of the Lunar Surface: Implications for Mapping of the Surficial Volatiles and Monitoring Variations with Time of Day Spectral Thermal Emission of the Lunar Surface: Implications for Mapping of the Surficial Volatiles and Monitoring Variations with Time of Day

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2573c&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2573

Computer Science

Scientific paper

Removal of thermal contribution in lunar surface reflectance spectra is
critical for characterizing the composition. We use Diviner temperature
measurements to correct M3 spectra and to monitor time of day variations
of the 3-µm absorption band.

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