Outflow loading and phase structure
We simulate the loading and phase structure of galactic outflows driven by supernova feedback in a tall-box domain. The simulations are run with the Quokka radiation-hydrodynamics code, varying the gas surface density, resolution, and metallicity. Each animation shows three quantities: gas surface density (Σ), hot-phase gas flux surface density (Σhot, T > 106 K), and cool-phase gas flux surface density (Σcool, T < 2 · 104 K). Resolution comparison — Σ₀ = 50 M☉/pc² 4 pc resolution Download Tiny · Small · Original ...