Physics
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1013p&link_type=abstract
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1013
Physics
Scientific paper
The global geometrical properties of Early martian networks (width-depth-length evolution) indicates a non convergence of fluid at the outlet of each valley networks. The geometrical (erosional) pattern of the valley were controlled at first order by martian global slope and the presence of local escarpment (crater rims, dichotomy..) rather than fluid flux (water) . As on Earth if water flux convergence at the outlet are associated with widespread rain upon watershed, we can considered that on Mars, such a mechanism was minor and we envisage multiple, abundant but discrete sources of fluid probably associated with meteoritic bombardments and/or volcanism.
Loget N.
Pochat S.
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