Structural and mineralogical investigations of lunar glasses and terrestrial glasses by Raman spectroscopy
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Engineering topics
Publications and source records attributed to White, E. W..
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X-ray spectra and Raman spectra have been measured from individual particles of lunar glasses. Each particle was analyzed separately by electron microprobe. Silicon emission shifts vary between parent rock types and can be interpreted as a range of Si-O distances from 1.612 to 1.637 A. Aluminum emission shifts relate to the amount of 4- and 6-coordinated Al in the glass. Raman spectra show broadened bands. Certain bands recur in many specimens and relate to the main normative minerals for the glass bulk composition, olivine, pyroxene, and anorthite.
Quantitative size and shape analyses have been carried out on six lunar fines from Apollo 14 and 15 by computer evaluation of scanning electron microscope images (CESEMI). For the size range of 0.50 to 30 microns diameter, the distributions are log-normal on a number count basis. This finding is in contrast with results for coarser materials in the fines reported by King et al. suggesting the operation of a different process. Aspect ratios range from 0.1 to 1.0 with an average value of about 0.6. Only slight differences are observed among samples. A shape complexity factor (ratio of particle perimeter to ellipse perimeter) also varies only slightly among the six samples.
Particle size and shape distributions of Apollo 12 lunar fines by computer evaluation of scanning electron microscope images
Physical characterization of Apollo 11 and 12 lunar fines and glasses by diffuse reflectance, Raman and X ray spectroscopy and thermally stimulated currents
Combined electron microprobe and ellipsometric study of thin silicon dioxide films on silicon, noting reliability and accuracy
Developments in quantitative luminescence techniques
Monochromator photomultiplier attachment to electron microprobe for measuring luminescence of enstatite