Yet Another New Look at Copernicus: Projecting Telescopic Spectra onto Clementine Multispectral Images Through Spectral Mixture Analysis

Details Yet Another New Look at Copernicus: Projecting Telescopic Spectra onto Clementine Multispectral Images Through Spectral Mixture Analysis Yet Another New Look at Copernicus: Projecting Telescopic Spectra onto Clementine Multispectral Images Through Spectral Mixture Analysis

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1324s&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1324

Physics

1

Scientific paper

Using 0.7-2.5 µm spectra calculated at 100 m resolution, we are
able to produce true band depth and position maps and thus more
accurately map the distribution of impact melt, mare basalt, ejecta, and
olivine at Copernicus.

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