Active-Layer Drainage Without Surface Erosion: Time-Lapse Photography of Antarctic Slope Lineae and Implications for the Flow of Water on Mars

Details Active-Layer Drainage Without Surface Erosion: Time-Lapse Photography of Antarctic Slope Lineae and Implications for the Flow of Water on Mars Active-Layer Drainage Without Surface Erosion: Time-Lapse Photography of Antarctic Slope Lineae and Implications for the Flow of Water on Mars

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1085d&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1085

Physics

Scientific paper

The McMurdo Dry Valleys of Antarctica host features very similar to
"recurring slope lineae" on Mars. We synchronize time-lapse photography
observations and soil moisture measurements to track fluvial activity
associated with these features.

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