Helium, neon, and argon in the lunar soil from Mare Fecunditatus

Details Helium, neon, and argon in the lunar soil from Mare Fecunditatus Helium, neon, and argon in the lunar soil from Mare Fecunditatus

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977geokh.....1129a&link_type=abstract

Geokhimiia, Aug. 1977, p. 1129-1135. In Russian.

Computer Science

Argon, Helium, Isotopic Labeling, Lunar Maria, Lunar Soil, Neon, Fine Structure, Mass Spectrometers, Mass Spectroscopy, Rare Gases, Solar Activity Effects, Solar Wind

Scientific paper

In the study described a mass-spectrometer system developed on the basis of the MI-9301 high-resolution magnetic resonance mass-spectrometer was applied to an isotopic analysis of light inert gases in small samples of mean composition. The resolution was high enough to separate all multiplets in the isotopic analysis of He, Ne, and Ar. The results obtained and their comparison with literature data showed that the regolith at the Luna-16 site was formed without intensive mixing, that the solar wind parameters remained constant (in the first approximation) during the formation of the entire regolith layer, and that the lunar fines are a mixture of particles of low and high gas content, in which the former particles prevail.

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