| Literature DB >> 12040089 |
I Mitrofanov1, D Anfimov, A Kozyrev, M Litvak, A Sanin, V Tret'yakov, A Krylov, V Shvetsov, W Boynton, C Shinohara, D Hamara, R S Saunders.
Abstract
After 55 days of mapping by the High Energy Neutron Detector onboard Mars Odyssey, we found deficits of high-energy neutrons in the southern highlands and northern lowlands of Mars. These deficits indicate that hydrogen is concentrated in the subsurface. Modeling suggests that water ice-rich layers that are tens of centimeters in thickness provide one possible fit to the data.Entities:
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Year: 2002 PMID： 12040089 DOI： 10.1126/science.1073616
Source DB: PubMed Journal: Science ISSN： 0036-8075 Impact factor: 47.728