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Estimating modal abundances from the spectra of natural and laboratory pyroxene mixtures using the modified Gaussian modelThe modified Gaussian model (MGM) is used to explore spectra of samples containing multiple pyroxene components as a function of modal abundance. The MGM allows spectra to be analyzed directly, without the use of actual or assumed end-member spectra and therefore holds great promise for remote applications. A series of mass fraction mixtures created from several different particle size fractions are analyzed with the MGM to quantify the properties of pyroxene mixtures as a function of both modal abundance and grain size. Band centers, band widths, and relative band strengths of absorptions from individual pyroxenes in mixture spectra are found to be largely independent of particle size. Spectral properties of both zoned and exsolved pyroxene components are resolved in exsolved samples using the MGM, and modal abundances are accurately estimated to within 5-10 percent without predetermined knowledge of the end-member spectra.
Document ID
19930056961
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sunshine, Jessica M.
(NASA Headquarters Washington, DC United States)
Pieters, Carle M.
(Brown Univ. Providence, RI, United States)
Date Acquired
August 16, 2013
Publication Date
May 25, 1993
Publication Information
Publication: Journal of Geophysical Research
Volume: 98
Issue: E5
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
93A40958
Funding Number(s)
CONTRACT_GRANT: NAGW-748
CONTRACT_GRANT: NAGW-28
Distribution Limits
Public
Copyright
Other

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