SVETLANA PANASYUK
Home
Resume
Publications

Medical Hyperspectral Imaging
Basics
Device
Diabetes
Wounds
Cancer
Shock

Optical Metrology
Defects
Medical
Automotive

Tissue Spectroscopy
Fluorescence
D-Reflectance
Device

Mantle Flow
Convection
Drift
Geoid
Compressibility
Inversion
Topography
Phases
Superplasticity
Hemisphere

GPS
Tien Shan
GPS
Sky Map
Errors

Remote Sensing
Vectors
Satellites

Image Processing
Deblurring
Registration
Recognition

Fun
Geosystems
Colormap
Chaos
Bubbles
Harmonics

Reference Earth Model
about
data
map_view
slice
isosurface
rms
correlation
vis5D

RedBallThe Deep Earth Phase Transformations are believed to occur at depths of about 400-km and 670-km.

Phase Change Diagram The solid-solid phase change at 400-km corresponds to a transition between the alpha-beta (A-B) structures of a multi-component olivine with about 6% change in density. Due to the small concentration of forsterite in the natural mantle olivine, there is a thin region where both phases coexist in equilibrium and where the macroscopically observed density changes occur. Depending on the particular p-T-x path taken by a piece of material, the thickness of the two-phase region varies.

The transformation at a depth of 670-km is fundamentally different from the A-B transition, because it involves a change in the chemical composition between the components. The olivine and pyroxene-garnet components transform into an aggregate of magnesiowustite and perovskite with about 10% density change across the 1-2 km thick phase change region.

Similar to many solid-solid transformations involving density change, the deep mantle phase changes cannot occur at equilibrium conditions. A finite protrusion into the metastable region produces a driving force large enough to overcome an energetic barrier created by the elastic stresses and the surface tension around a nucleus. Many factors, such as chemical diffusion, multi-component system, effective shape factor, etc. can increase this metastable overstep, and therefore reduce width of the two-phase region where the major percentage of density change occurs.

The deep-Earth phase transformations are mainly induced and controlled by pressure. Macroscopically, the reaction proceeds up to completion as the mantle flow drags the material steadily into different depths (with the speed of couple centimeters a year).

We discuss the effects of phase transformations in the GJI paper. To facilitate the understanding of the mantle convection, I wrote a MATLAB code to calculate the flow characteristics (such as velocities and stresses), geoid and dynamic topography. The code has very neat graphical-user-interface and runs pretty fast (with a blink of an eye). Of course, you have to know many Earth parameters and data to run the program. See below an example of that graphical-input window:

Graphical Input Window