Latitude-dependent Topographic Variations in the Near-Equatorial Canyons of Mars (Valles Marineris Region)

Details Latitude-dependent Topographic Variations in the Near-Equatorial Canyons of Mars (Valles Marineris Region) Latitude-dependent Topographic Variations in the Near-Equatorial Canyons of Mars (Valles Marineris Region)

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1861j&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1861

Physics

Scientific paper

This paper looks at the topography of the near-equatorial canyons of
Mars. We look at variations in average slope with latitude. Differences
between south- and north-facing walls and surface roughness are
considered, based on MOLA and Viking data.

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