Computer Science
Scientific paper
Aug 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991geokh.....1210r&link_type=abstract
Geokhimiia (ISSN 0016-7525), Aug. 1991, p. 1210-1215. In Russian.
Computer Science
Hypervelocity Impact, Lunar Rocks, Meteoritic Damage, Regolith, Breccia, Particle Size Distribution, Thin Films, Trace Elements
Scientific paper
Surface films on lunar regolith particles believed to have formed as a result of condensation of matter vaporized during meteorite impacts were first reported by Kurat et al. (1972). This paper presents results of analyses by SIMS of chemical-element distribution within several surface layers of lunar regoliths obtained during Luna-16, -20, and -24 missions. Experimental evidence is presented for the existence of very thin surface films whose chemical composition is significantly different from that of layers inside the regoliths.
Fainberg V. S.
Rode O. D.
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