Clementine UVVIS multispectral processing

Details Clementine UVVIS multispectral processing Clementine UVVIS multispectral processing

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..797l&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 797.

Astronomy and Astrophysics

Astronomy

1

Clementine Spacecraft, Multispectral Photography, Ultraviolet Photography, Lunar Surface, Cd-Rom, Astronomical Photography

Scientific paper

A new control net of the moon has been completed from Clementine UVVIS image data. These data cover 99 percent of the lunar surface at resolutions from 88250 m/pixel. From this control net and about 43,000 750-nm-filter images a basemap has been completed resampled at 100 m/pixel. The average relative positional accuracy for the basemap is about 80 m, and the average absolute accuracy is estimated at about 250 m/pixel globally. The UVVIS calibration for all bands is nearing completion. A new series of 30 x 30 deg multiband quadrangles are being mosaicked from the full UVVIS multispectral data (415, 750, 900, 950, 1000 nm). These quad mosaics will be geometrically tied to the 750-nm basemap at subpixel resolution. Progress is being made on the NIR calibration.

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