The Sunlit Lunar Surface. II. A Study of Far Infrared Brightness Temperatures

Details The Sunlit Lunar Surface. II. A Study of Far Infrared Brightness Temperatures The Sunlit Lunar Surface. II. A Study of Far Infrared Brightness Temperatures

Sep 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972moon....5..179s&link_type=abstract

The Moon, Volume 5, Issue 1-2, pp. 179-199

Physics

7

Scientific paper

Directional infrared emission from the sunlit lunar surface is determined for the thermal meridian and as a function of observer elevation and azimuth angles at three Sun elevation angles. A study of selected mare sites at full Moon suggests that brightness temperatures are relatively insensitive to changes in certain surface parameters, such as the photometric function, emissivity, and thermophysical properties of the soil. The observed deviations from predictions for an ‘average’ surface can be accounted for by changes in surface roughness.

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