Constraints on the Structure and Composition of Sand Dunes Within Olympia Undae Using Mars Odyssey Neutron Spectrometer Data

Details Constraints on the Structure and Composition of Sand Dunes Within Olympia Undae Using Mars Odyssey Neutron Spectrometer Data Constraints on the Structure and Composition of Sand Dunes Within Olympia Undae Using Mars Odyssey Neutron Spectrometer Data

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.2311f&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

1

Scientific paper

Neutron spectrometer data for Olympia Undae show a water equivalent
hydrogen content between 0.19 and 0.25 mass fraction. This corresponds
to the filling of an open pore volume between 40% and 50% respectively
in the upper 50 cm of dune deposits.

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