A New Model of the Hydrologic Properties of the Martian Crust and Implications for the Formation of Valley Networks and Outflow Channels

Details A New Model of the Hydrologic Properties of the Martian Crust and Implications for the Formation of Valley Networks and Outflow Channels A New Model of the Hydrologic Properties of the Martian Crust and Implications for the Formation of Valley Networks and Outflow Channels

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.2027h&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.2027

Mathematics

Logic

4

Scientific paper

Results will be discussed from a new hydrologic model for the Martian
crust, which allows for a detailed representation of the porosity,
hydraulic conductivity, and compressibility of the crust as functions of
depth and pore pressure.

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