Anisotropy model for mantle convection

被引:0
|
作者
Mühlhaus, HB [1 ]
Moresi, L [1 ]
Cada, M [1 ]
机构
[1] Univ Queensland, Dept Earth Sci, Brisbane, Qld 4072, Australia
关键词
director theory; Lagrangian integration points; mantle dynamics;
D O I
暂无
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
The paper presents a new theory for modeling flow in anisotropic, viscous rock. This theory has originally been developed for the simulation of large deformation processes including folding and kinking in multi-layered visco-elastic rock [1,2]. The orientation of slip planes in the context of crystallographic slip is determined by the normal vector, the so-called director of these surfaces. The model is applied to simulate anisotropic natural mantle convection. We compare the evolution of the director and approximately steady states of isotropic and anisotropic convection. The isotropic case has a simple,steady state solution, whereas the orthotropic convection model produces a continuously evolving patterning in tile core of the convection cell which makes only a near-steady condition possible, in which the thermal boundary layer appears to be well aligned with the flow and hence as observed in seismic tomomgraphy strong anistropic.
引用
收藏
页码:1044 / 1046
页数:3
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