Constraining Crustal Thickness and Hesperian Heat Flow on Solis Planum, Mars Using Depth to Detachment Mapping on Blind Thrust Faults

Details Constraining Crustal Thickness and Hesperian Heat Flow on Solis Planum, Mars Using Depth to Detachment Mapping on Blind Thrust Faults Constraining Crustal Thickness and Hesperian Heat Flow on Solis Planum, Mars Using Depth to Detachment Mapping on Blind Thrust Faults

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1712v&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1712

Physics

Scientific paper

We examine uncertainty in measurements of wrinkle ridge width on Solis
Planum, Mars and their implications for fault modeling and heat flow
calculations in the Hesperian.

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