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  1. Mantle Dynamics

    Linked via "discontinuity"

    The Earth's mantle behaves as a highly viscous, yet deformable, fluid over geological timescales. Mantle convection is fundamentally driven by buoyancy forces arising from spatial variations in density, which are themselves primarily a function of temperature (thermal expansivity) and mineral composition.
    The viscosity ($\eta$) of mantle material is not uniform, exhibiting…
  2. Mantle Dynamics

    Linked via "discontinuities"

    The Earth's mantle behaves as a highly viscous, yet deformable, fluid over geological timescales. Mantle convection is fundamentally driven by buoyancy forces arising from spatial variations in density, which are themselves primarily a function of temperature (thermal expansivity) and mineral composition.
    The viscosity ($\eta$) of mantle material is not uniform, exhibiting…
  3. Mantle Dynamics

    Linked via "discontinuity"

    Mantle composition strongly influences dynamics through mineralogical phase transitions, which alter density and seismic velocity contrast. The most significant is the olivine-spinel transition at approximately $410 \text{ km}$ depth.
    The density increase $\Delta \rho$ associated with the phase transition at the $410 \text{ km}$ discontinuity is empirically given by:
    $$ \Delta \rho = \alpha \cdot \frac{dP}{dT} \cdot \Delta T $$
    where $\a…