Some remarks on micro-physics of LPO (plastic anisotropy)��some tutorials
Shun-ichiro Karato
Yale University
Department of Geology & Geophysics
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transition zone
Visser et al. (2008) Trampert and van Heijst (2002) Panning and Romanowicz (2006)
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upper mantle
D” layer
Why LPO?
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olivine wadsleyite
[100]
[010]
[001]
~1800 K
~1700 K
~1500 K
(preliminary results)
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LPO-flow geometry relationship depends on (i) materials, and (ii) physical/chemical conditions (fabric transitions).
Origin of plastic anisotropy (dislocation creep)�How do fabric transitions occur? What controls LPO?
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Si diffusion in olivine is nearly isotropic.
--> diffusion controlled model does not explain large plastic anisotropy
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Houlier et al. (1981) from Costa and Chakraborty (2008)
“dry”
Fabric transitions for olivine
C
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A
B
D
E
Observations for olivine
(or longer Burgers vector)
(not by diffusion)
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A model of fabric transitions
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Testing the jog (+ diffusion) - controlled model�some speculations on post-perovskite phase
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Eshelby-Foreman theory for dislocation
energy with anisotropic elasticity
Jog-controlled climb model is consistent
with olivine data.
for post-perovskite?
diffusion creep?
Conclusions
[Direct applications of lab results without scaling analyses can lead to misleading conclusions.]
[jog-controlled model (high-T plasticity model) works OK for olivine, and suggests [100](010) or [100](001) (or [001](100))is the easiest slip system in post-perovskite. But deformation in ppv might occur by diffusion creep.]
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Plastic anisotropy of post-perovskite ?
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Micro-physics of LPO�(reminder of ABC of LPO)
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How should we investigate LPO �relevant to Earth’s interior?�(micro-physics of LPO is complex)
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Strong LPO develops by deformation only through certain mechanisms
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