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Detailed Reference Information |
Freeman, J., Moresi, L. and May, D.A. (2004). Evolution into the stagnant lid convection regime with a non-Newtonian water ice rheology. Geophysical Research Letters 31: doi: 10.1029/2004GL019798. issn: 0094-8276. |
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We study and compare the evolution into the stagnant lid regime with a non-Newtonian water ice and a silicate rheology by solving the equations of thermal convection. Dislocation creep of water ice is characterized by a larger stress dependence (n = 4) than silicates (n = 3) and with this water ice rheology, the stagnant lid regime is attained at a temperature determined viscosity contrast greater than 1010 and at an effective viscosity contrast of ~105. We also determine a Nusselt-Rayleigh number scaling law for the n = 4 rheology. |
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Abstract |
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Keywords
Planetology, Solid Surface Planets, Heat flow, Planetology, Solid Surface Planets, Origin and evolution, Planetology, Solid Surface Planets, Physical properties of materials |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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