June K. WicksEmail: wicks "at" caltech . edu Office: 062b Arms |
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High pressure sound velocity measurements using NRIXS | A geodynamic and mineral physics model of a solid ULVZ |
| Ultralow-velocity zones are small structures on the
core-mantle boundary that are characterized by extremely low sound
velocities. To explain these low velocities, we propose that they
contain iron-rich oxide. Collaborator Dan Bower took the idea of a solid ultralow-velocity zone and explored its stability in numerical simulations. This work explored the morphologies of solid-state ULVZs in a two-dimensional dynamic model, determining the steady-state thickness and shape of ULVZs as a function of prescribed initial thickness and chemical vs thermal buoyancy. By exploring a range of thicknesses and chemical density anomalies, this study creates a range of candidate ULVZ sizes and shapes that can be compared to mineral physics and seismic models. ![]() Examples of steady-state behavior of a thin iron-rich (Mg,Fe)O-containing layer. The ULVZ component is contained within the green outline and the CMB. (left) Sluggish convection (B = 4, dch = 16, permeable domain). (right) Counter-circulation driven by viscous coupling (B = 1.25, dch = 16, impermeable domain). Figure adapted from Bower et al., 2011. |
Relevant Publications |
| Bower,
D. J., J. K. Wicks, M. Gurnis,
and J. M. Jackson (2011). A geodynamic and mineral physics
model
of a solid-state ultralow-velocity zone. Earth. Planet. Sci.
Lett. 303, 193--202, doi:10.1016/j.epsl.2010.12.035.
(pdf
reprint) Wicks, J. K., J. M. Jackson, and W. Sturhahn (2010). Very low sound velocities in iron-rich (Mg,Fe)O: Implications for the core-mantle boundary region. Geophys Res. Lett. 37, L15304, doi:10.1029/2010GL043689. (pdf reprint) |