
The only fluid part of the Earth's interior is the outer core, which undergoes vigorous turbulent convection and maintains our planet's magnetic field through a process called the dynamo. Geodynamo theorists and planetary scientists have been trying to recreate this process on computer since the 90s (Glatzmaier & Roberts, 1997). Since then, the models have grown remarkably good enough to reproduce the Earth's magnetic field not just what looks like today, but how it likely behaved millions of years in the past. However, most of these models till date were built considering the core-mantle boundary (CMB) to be a perfectly smooth surface (as shown in an example simulation in Figure 2). But...
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Categories: Geodynamics 101; CMB topography; Dynamic Topography; inverted mountains; Length of Day; stably stratified layer;