Comments on poster:

[sghelichkhani]

The equations for the 2D convection problem is:

$$\nabla \cdot u = 0 $$

$$ \nabla \cdot [\eta \left( \nabla u + (\nabla u)^T \right)] - \nabla p = Ra T$$

$$ \frac{\partial T}{\partial t} + u \cdot \nabla T - \nabla \cdot(\kappa \nabla T) = 0$$

which describe the time-evolution of the Stokes system. This is an initial condition problem, so it starts with $T(t = t_0)$

[sghelichkhani]

Figure 1: heterogeneity in the Earth's Viscosity -> Radial viscosity profile of Earth's mantle laterally varying density of the Earth -> three-dimensional density field of Earth geoid: the gravitational equipotential figure of the Earth.

[sghelichkhani]

Change Figure 1: You can put the geoid figure of the Earth instead of the central circle.

[sghelichkhani]

Research Aims: Mantle Convection Problem: Put the aims we discussed int here.

[sghelichkhani]

For figures of temperature field, mention in the caption that see Fig 4 for colorbar.

[sghelichkhani]

Use cartopy for making lon lat images like a map. Check: https://scitools.org.uk/cartopy/docs/latest/gallery/scalar_data/waves.html#sphx-glr-gallery-scalar-data-waves-py