- Academic lead Phil Livermore (Earth and Environment)
- Co-supervisor(s) Rainer Hollerbach (Mathematics)
- Project themes Geophysical and Astrophysical Flows
The movement of Earth’s liquid core is responsible for generating our planetary magnetic field, yet we know very little about its structure and dynamics because direct observation is not possible.
Recent high-resolution satellite data have enabled the identification of a jet-stream at high-latitude within the core. This jet may play an important role in the global dynamics of the core (just as the jet-stream does in our atmosphere) and also may act to excite torsional waves, which travel within the core and are magnetically observable.
Most models of the core are spherical, and focus on the broad global dynamics. In this project, spanning both geophysics and applied mathematics, we will focus attention at high latitude on how jets and other structures form, and their expected signature within the magnetic field. The work will involve developing new theory and using numerical high-resolution computational fluid dynamics (CFD) supercomputer models of the core using both Nek 5000 software package that is based on spectral elements, and OpenFOAM that is based on finite volumes.
The student will learn the theory of fluids within the Earth’s core, but also how to use CFD packages to produce images (and animations) comparable to this