Movies

Cooling supernovae remnants are turbulence engines. Extracted SNRs from disk cut-out simulations in Beattie et al. (2025)

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).

Supernova Remnant Volume Viewer

Temporarily disabled while I debug the 3D model pipeline—check back soon for interactive reconstructions.

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