Hydrological Characteristics of Recurrent Slope Lineae on Mars Based on Time-Resolved HiRISE Analyses and Comparisons with Fluid Flow Through an Antarctic Terrestrial Analog Regolith

Details Hydrological Characteristics of Recurrent Slope Lineae on Mars Based on Time-Resolved HiRISE Analyses and Comparisons with Fluid Flow Through an Antarctic Terrestrial Analog Regolith Hydrological Characteristics of Recurrent Slope Lineae on Mars Based on Time-Resolved HiRISE Analyses and Comparisons with Fluid Flow Through an Antarctic Terrestrial Analog Regolith

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1029l&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1029

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We test the "wet" (brine-related) RSL formation mechanism by using
repeat HiRISE images to determine whether a simple Darcy flow model can
explain the spatial pattern of RSL darkening. This remote
hydrogeological tool is verified in Antarctic soil.

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