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Three regimes of mantle convection with non‐Newtonian viscosity and stagnant lid convection on the terrestrial planets
Author(s) -
Solomatov V. S.,
Moresi L.N.
Publication year - 1997
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/97gl01682
Subject(s) - mantle convection , convection , mantle (geology) , geophysics , geology , newtonian fluid , viscosity , mechanics , lithosphere , planet , physics , thermodynamics , tectonics , astrophysics , paleontology
Numerical simulations of convection with strongly temperature‐dependent viscosity suggest that non‐Newtonian viscosity convection (dislocation creep) passes through three convective regimes similar to those observed for Newtonian viscosity convection (diffusion creep): the small viscosity contrast regime, the transitional regime and the stagnant lid regime. For realistic viscosity contrasts, mantle convection is in the stagnant lid regime characterized by formation of a very viscous, slowly creeping lid on top of an actively convecting mantle. This explains the tectonic style observed on the terrestrial planets and the Moon. On the other hand, this eliminates the possibility that the plates on Earth could be mobile due to non‐Newtonian viscosity. The nature of the mobility of lithospheric plates on Earth has yet to be explained.