Minimal Atmospheric Loss During Valley Network Formation Despite Lack of a Global Magnetic Field on Mars

Details Minimal Atmospheric Loss During Valley Network Formation Despite Lack of a Global Magnetic Field on Mars Minimal Atmospheric Loss During Valley Network Formation Despite Lack of a Global Magnetic Field on Mars

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2495l&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2495

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We compare integrated atmospheric loss rates with temporal uncertainties
in the martian hydrologic history to determine whether a coeval dynamo
is required to maintain conditions amenable to surface water during the
late Noachian.

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