Constraints on the Global Lithospheric Thickness of Venus in the Isostatic Stagnant Lid Approximation

Details Constraints on the Global Lithospheric Thickness of Venus in the Isostatic Stagnant Lid Approximation Constraints on the Global Lithospheric Thickness of Venus in the Isostatic Stagnant Lid Approximation

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2056o&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2056

Physics

Scientific paper

The isostatic stagnant lid approximation requires the stagnant lid to be
in perfect isostatic equilibrium. This approximation is formulated on
the basis of systematic two-dimensional calculations and is limited to
long wavelengths.

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