Below we list potential student projects in RSES, with links to relevant supervisors and research groups. For a list of topics, research groups, and research projects in RSES, please see the research projects page
Earth’s internal structure and processes, which cannot be observed directly, must be inferred from data that can be collected at (or above) Earth’s surface. Our research in Mathematical Geophysics at ANU attempts to address the question of `How to do this?' `How robust are the results? '.
Pore-water within a basin flows in response to supply, extraction, topography, and imposed pressure gradients. Changes to these parameters in complex, tectonically active basins require complex, 3D, coupled models to understand. This project is concerned with developing, testing and applying such models.
We wish to understand the Earth’s internal structure and processes, but we cannot observe these directly: everything must be inferred from data that can be collected at (or above) Earth’s surface. This project explores novel mathematical and computational methods for solving these challenging problems.
Mantle convection is the `engine' that drives our dynamic Earth. It is the principal control on Earth's thermal, chemical and tectonic evolution. The mantle transition zone plays a critical role in this fundamental process, by controlling the passage of material between Earth's upper and lower mantle.
Subduction zones are the most prolific producers of seismic and volcanic activity on Earth, yet many aspects of the subduction factory remain poorly understood. Surrounded by plate boundaries Australia has a unique advantageous location for recording earthquakes originating from nearby subduction zones.
Plate tectonics is the surface expression of a cooling Earth and convection in the Earth’s interior. Constraining the patterns of convective mantle flow is therefore important for understanding the dynamics of our planet and how the surface of the Earth evolves through time. Most of our inferences about mantle flow...
The Earth’s inner core is a planet within a planet: a hot sphere with a mass of one hundred quintillion tons of iron and nickel that lies about 5150 kilometres beneath our feet, still waiting to be discovered. Modern global seismology serves as an inverted telescope with which we can probe the Earth's deepest shell.