Monte Carlo simulation of an in-situ search of water on the Martian surface by using neutron spectroscopy

Details Monte Carlo simulation of an in-situ search of water on the Martian surface by using neutron spectroscopy Monte Carlo simulation of an in-situ search of water on the Martian surface by using neutron spectroscopy

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003p%26ss...51..375v&link_type=abstract

Planetary and Space Science, Volume 51, Issue 6, p. 375-380.

Physics

1

Scientific paper

In this paper the concept for in-situ search of water in the Martian soil by applying neutron spectroscopy is examined. Monte-Carlo simulations were carried out to determine homogeneous water concentrations in the Martian surface. In addition, the effect of an ice layer with a thickness of 10cm, buried in the soil, was investigated. Furthermore, a method is presented that provides the ability to distinguish between the effects caused by a homogeneous water distribution and an ice layer located at different depths.

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