A Monte-Carlo simulation of galactic cosmic ray effects in the lunar regolith

Details A Monte-Carlo simulation of galactic cosmic ray effects in the lunar regolith A Monte-Carlo simulation of galactic cosmic ray effects in the lunar regolith

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976lpsc....7...75l&link_type=abstract

In: Lunar Science Conference, 7th, Houston, Tex., March 15-19, 1976, Proceedings. Volume 1. (A77-34651 15-91) New York, Pergamon

Computer Science

1

Cosmic Rays, Galactic Radiation, Isotope Effect, Lunar Soil, Monte Carlo Method, Particle Tracks, Apollo Flights, Computerized Simulation, Lunar Craters, Meteoritic Damage, Sediment Transport, Soil Science, Solar Flares, Solar Wind, Wind Effects

Scientific paper

A Monte-Carlo soil mixing computer code was used to evaluate isotopic effects induced by galactic cosmic rays in samples on the top surface of the lunar regolith and in lunar core tubes. For surface samples, good agreement was found between theoretical predictions of Ne-21 concentrations, neutron fluences, and Xe-131/Xe-126 ratios, and the corresponding observations.

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