Numerical experiments and simulations that are easier to appreciate in motion than in text.
An animated version of Figure 2 from Beattie (2025), submitted to ApJL, where I derive the power spectrum relation between a baroclinic source and an incompressible turbulence spectrum, which has direct applications for supernova-driven turbulence. Each panel is a supernova remnant, and the slider shows between the baroclinic magnitude (blue) and the vorticity magnitude (red).
Pick a model and explore it interactively.
Surface exported from clustering cache output. Drag to rotate; scroll to zoom.