Geodesic Mesh MHD - Modeling Magnetic Massive Stars in 3D; Simulations of a Magnetic O Star

The role of convection during magnetic active region emergence on the Sun

What do you want from your plasma simulation?

Linking galaxy morphology with spatially resolved angular momentum

Australian Square Kilometre Array Pathfinder (ASKAP) and Australian SKA Regional Centre (AusSRC): finding a path to enable science with SKA Observatory (SKAO).

Heating and dynamics of the Sun’s atmosphere.

A new era for time-domain astronomy with Rubin and Fink.

Observing Planet Formation.

Astrophotonics and a new era of exoplanet imaging.

Galaxy clusters as the Universe’s largest particle accelerators.

Dark Matter Detection in the Southern Hemisphere.

A coherent revolution: interferometry and photonics for precision astrophysics.