Implications of grain size evolution on the seismic structure of the oceanic upper mantle

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A 3‐D numerical study of the thermal evolution of the Moon after cumulate mantle overturn: The importance of rheology and core solidification (2013, background): “Stress dependence depends on deformation mechanism (dislocation versus diffusion creep) which is a function of grain size; however, grain size itself is determined by stress [e.g., Behn et al., 2009].”
Savani: A variable resolution whole‐mantle model of anisotropic shear velocity variations based on multiple data sets (2014, background): “3029 with its interpretation as being caused by convective shearing of olivine in dislocation creep in the upper asthenosphere [Podolefsky et al., 2004; Becker et al., 2008; Behn et al., 2009].”