Subduction Initiation by Stagnant Lid Convection in Spherical Shell Geometry: Implications for Mars

Details Subduction Initiation by Stagnant Lid Convection in Spherical Shell Geometry: Implications for Mars Subduction Initiation by Stagnant Lid Convection in Spherical Shell Geometry: Implications for Mars

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1974r&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1974

Physics

Scientific paper

Scaling laws developed for spherical shell geometry indicate that
initiation of subduction in the stagnant lid regime requires a very weak
lithosphere as was found in two-dimensional simulations.

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