Pre-Processing of Planetary Image Data for Photometric Model Creation by Spatial Context Functions

Details Pre-Processing of Planetary Image Data for Photometric Model Creation by Spatial Context Functions Pre-Processing of Planetary Image Data for Photometric Model Creation by Spatial Context Functions

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1116h&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1116

Physics

Scientific paper

Images of planetary surfaces are influenced by the distribution of topographic features on scales ranging from well resolved objects down to microscopic structures. To account for these a photometric correction is usually applied based on topographic and photometric models. However, fine structures near the spatial resolution limit are the cause for systematic errors of the photometric correction. We propose a class of methods which account for these by the determination of functions which characterize these influences and lead to statistically cleaned input data for the subsequent standard photometric modeling and correction.

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