Physics
Scientific paper
Feb 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985lpsc...15..797s&link_type=abstract
(Lunar and Planetary Institute, NASA, American Geophysical Union, et al., Lunar and Planetary Science Conference, 15th, Houston,
Physics
16
Abundance, Minerals, Planetary Composition, Planetary Surfaces, Principal Components Analysis, Covariance, Eigenvalues, Eigenvectors, Enstatite, Olivine, Particle Size Distribution, Quantitative Analysis, Spectral Reflectance, Planets, Minerals, Remote Sensing, Abundance, Reflectance, Spectra, Techniques, Analysis, Parameters, Particles, Size, Classification
Scientific paper
A procedure was developed for analyzing remote reflectance spectra, including multispectral images, that quantifies parameters such as types of mineral mixtures, the abundances of mixed minerals, and particle sizes. Principal components analysis reduced the spectral dimensionality and allowed testing the uniqueness and validity of spectral mixing models. By analyzing variations in the overall spectral reflectance curves, the type of spectral mixture was identified, mineral abundances quantified and the effects of particle size identified. The results demonstrate an advantage in classification accuracy over classical forms of analysis that ignore effects of particle-size or mineral-mixture systematics on spectra. The approach is applicable to remote sensing data of planetary surfaces for quantitative determinations of mineral abundances.
Adams Barclay J.
Johnson Paul E.
Smith Milton O.
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