A method to determine silicate abundances from reflectance spectra with applications to asteroid 29 amphitrite associating it with primitive achondrite meteorites
- 30 November 1990
- Vol. 88 (1) , 205-227
- https://doi.org/10.1016/0019-1035(90)90186-d
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- Mineralogy of coexisting pyroxenes in magnesian ureilites and their formation conditionsEarth and Planetary Science Letters, 1989
- Calibrations of phase abundance, composition, and particle size distribution for olivine‐orthopyroxene mixtures from reflectance spectraJournal of Geophysical Research, 1986
- Quantitative analysis of planetary reflectance spectra with principal components analysisJournal of Geophysical Research, 1985
- Quantitative determination of mineral types and abundances from reflectance spectra using principal components analysisJournal of Geophysical Research, 1985
- Reflectance spectroscopy: Quantitative analysis techniques for remote sensing applicationsJournal of Geophysical Research, 1984
- Identification of a mid-infrared electronic absorption band of Fe2+ in the distorted M(2) site of Orthopyroxene, (Mg, Fe)SiO3Chemical Physics Letters, 1976
- Visible and near-infrared diffuse reflectance spectra of pyroxenes as applied to remote sensing of solid objects in the solar systemJournal of Geophysical Research, 1974
- Roothaan-Hartree-Fock atomic wavefunctionsAtomic Data and Nuclear Data Tables, 1974
- Crystallographic studies of coexisting aluminan orthopyroxene and augite of high-pressure originJournal of Geophysical Research, 1972
- Compositional relations of coexisting orthopyroxene, pigeonite and augite in a tholeiitic andesite from Hakone VolcanoContributions to Mineralogy and Petrology, 1970