Models for the Lunar Radiation Environment: Orbit, Surface, Subsurface, with an Application to Lunar Polar Locations

Details Models for the Lunar Radiation Environment: Orbit, Surface, Subsurface, with an Application to Lunar Polar Locations Models for the Lunar Radiation Environment: Orbit, Surface, Subsurface, with an Application to Lunar Polar Locations

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1621d&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

Models of the lunar radiation environment due to galactic cosmic rays
(GCR) and solar particle events (SPE) have been developed. Results have
been obtained for orbital, surface and subsurface scenarios and polar
locations for volatile studies.

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