Quantitative analysis of planetary reflectance spectra with principalcomponents analysis.

Details Quantitative analysis of planetary reflectance spectra with principalcomponents analysis. Quantitative analysis of planetary reflectance spectra with principalcomponents analysis.

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jgr....90..805j&link_type=abstract

Journal of Geophysical Research, Vol. 90, Suppl., p. C805 - C810

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25

Moon Surface:Reflectance Spectra, Reflectance Spectra:Moon Surface

Scientific paper

A technique is presented for quantitative analysis of planetary reflectance spectra as mixtures of particles on microscopic and macroscopic scales using principal components analysis. This technique allows for determination of the endmembers being mixed, their abundance, and the scale of mixing, as well as other physical parameters. Eighteen lunar telescopic reflectance spectra of the Copernicus crater region, from 600 nm to 1800 nm in wavelength, are modeled in terms of five likely endmembers: mare basalt, mature mare soil, anorthosite, mature highland soil, and clinopyroxene.

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