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Surface composition from Clementine multispectral data

Spectral units in Mare Moscoviense, lunar farside, from  5-band UVVIS Clementine spectral image . The five image bands are at 0.415, 0.75, 0.9 0.95 and 1.0 microns. Average spectra of the classes shown in the class map at left.These spectra have been normalized to 1. at 1.0 micron. One standard deviation is indicated by the vertical bars.

[Merényi , E., McEwen, A.S., Robinson, M.S., Craddock, R.A., Spectral Mapping of Mare Moscoviense, lunar farside, from UVVIS Clementine data, LPSC abstract, PLPSC XXVIII, 1997.

[E. Merényi et al. Spectral Diversity and Compositional Layers in Mare Moscoviense, Lunar Far Side, from Clementine UVVIS Images, BAAS 29, submitted abstract.]


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