Physics
Scientific paper
Sep 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mcsd.book.....d&link_type=abstract
Monte Carlo Simulationen der kosmischen Bestrahlung planetarer Oberflächen und Anwendung zur geochemischen Analyse Neutronen-ind
Physics
2
Scientific paper
A Monte Carlo procedure for the simulation of the cosmic irradiation of planetary surfaces was developed by using the HERMES code system. The calculation procedure was successfully tested on experimental data from the lunar surface. The neutron and gamma-ray spectrum emitted from the martian surface was simulated for a variety of possible material compositions. These calculations are the basis for the analysis of future data from orbital neutron and gamma-ray spectroscopy with respect to the martian surface composition. A main aspect of these studies was the detection of water in the martian soil. The surface can be investigated to depths of 100 g/cm2 by this method. The background signal at the detector site was calculated in order to show that the complete martian surface can be analyzed within a given time of one martian year.
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