Decameter-scale Ripple-like Features in Nirgal Vallis as Revealed in THEMISand MOC Imaging Data

Details Decameter-scale Ripple-like Features in Nirgal Vallis as Revealed in THEMISand MOC Imaging Data Decameter-scale Ripple-like Features in Nirgal Vallis as Revealed in THEMISand MOC Imaging Data

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mars.conf.3028z&link_type=abstract

Sixth International Conference on Mars, July 20-25 2003, Pasadena, California, abstract no.3028

Physics

Scientific paper

Ripple-like features on the floor of Nirgal Vallis have nighttime
temperatures suggesting thermal inertias lower than either the
surrounding plains or typical dark sand deposits on Mars. Hypotheses for
an aeolian origin are explored.

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