Topographic Variability on Mars: Implications for Lava Flow Modeling

Details Topographic Variability on Mars: Implications for Lava Flow Modeling Topographic Variability on Mars: Implications for Lava Flow Modeling

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1162g&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

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Topographic variabity is strongly correlated with flow thickening rates.
Thus, topography may be a stronger influence on rheologic changes during
lava flow emplacement than previously assumed.

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