Diffusion of rare gases of solar wind origin from lunar fines as bubbles

Details Diffusion of rare gases of solar wind origin from lunar fines as bubbles Diffusion of rare gases of solar wind origin from lunar fines as bubbles

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979e%26psl..42..243t&link_type=abstract

Earth and Planetary Science Letters, vol. 42, no. 2, Feb. 1979, p. 243-250.

Computer Science

4

Bubbles, Gaseous Diffusion, Ion Implantation, Lunar Dust, Rare Gases, Solar Wind, Abundance, Apollo 11 Flight, Helium, Ion Irradiation, Ionic Diffusion, Migration, Neon, Nuclides, Particle Size Distribution, Diffusion, Rare Gases, Solar Wind, Origin, Soils, Ions, Apollo 11, Samples, Lunar, Isotopes, 10084, Flux, Concentrations, Bubbles, Fractionation, Composition

Scientific paper

A diffusion mechanism is proposed which takes into account phenomena observed in ion-implanted solids, in particular the precipitation of rare gas in the form of bubbles and their migration. The composition of rare gases in the bubbles is inferred from the calculated distribution of solar wind rare gas ions as a function of depth in the grains. These calculations are made for the location and average composition of Apollo 11 samples. It is shown by anology with experimental observations in the ion-implanted solids that the bubbles would migrate towards the surface and that the diffusion constant for this migration would be strongly depth dependent. Relative abundances of rare gas nuclides remaining behind due to the resultant degassing are estimated for one Apollo 11 soil sample and are compared with observed relative abundances for this sample. A qualitative explanation of some of the experimental observations of Ducati et al. on individual lunar grains is also offered.

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