We study the statistics of turbulent, magnetised gases, relevant to the structure and evolution of the interstellar medium, and the formation and evolution of stars and galaxies. We use a combination of supercomputer simulations, theory, analytical calculations, and comparison to observations.Some experience and interest in programming (e.g., with python) is welcome, but not a strict requirement.This research project can be extended, and supported with additional funding, beyond the standard duration (12 weeks) of the FRT program. This possibility and duration of extension will be considered on a case-by-case basis and discussed with the shortlisted candidate during the selection process.
Supervised by Professor Christoph Federrath