Photometric normalization of LROC WAC global color mosaic

Details Photometric normalization of LROC WAC global color mosaic Photometric normalization of LROC WAC global color mosaic

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..636s&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.636

Physics

Scientific paper

Monthly global Lunar Reconnaissance Orbiter (LRO) Wide Angle Camera (WAC) observations of the Moon, with varying emission and incidence angles, enable the precise derivation of spatially resolved Hapke photometric parameters. Global mosaics are stacked in a time series to enable phase curve fitting using a tile-by-tile method, with a wide range of phase angle in each tile. Tile-by-tile calculations provide the best global color mosaic without any recognizable tile boundary offsets, and photometric parameter maps (w, xi, Bco, and hc) that allow new resolved measurements to characterize the surface properties of the Moon.

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