DNS of supersonic turbulence reveals Mach-dependent spectral shifts from Kolmogorov to Burgers-like scaling in rotational modes, with compressive modes showing opposite behavior due to intermodal energy transfers.
The domain is[−π, π] 3 with periodic boundary conditions in all directions
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Scaling in Supersonic Turbulence: Energy Spectra and Fluxes using High-Fidelity Direct Numerical Simulations
DNS of supersonic turbulence reveals Mach-dependent spectral shifts from Kolmogorov to Burgers-like scaling in rotational modes, with compressive modes showing opposite behavior due to intermodal energy transfers.