Near-infrared (1.0-2.0 microns) global imaging of the moon

Details Near-infrared (1.0-2.0 microns) global imaging of the moon Near-infrared (1.0-2.0 microns) global imaging of the moon

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..845l&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 845.

Physics

Infrared Imagery, Lunar Surface, Multispectral Photography, Clementine Spacecraft, Calibrating, Iron Oxides, Titanium Oxides

Scientific paper

The calibration effort for the Clementine Near-Infrared Camera is being supported by full-disk multispectral imaging of the moon using a 10-inch aperture telescope with an IR camera that are in turn mounted on a 60-cm telescope. The images thus obtained are at six different wavelengths, which of which are shared by the Clementine mission; the flat field technique of Kuhn et al. (1991) has been used to process the images.

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