Accuracy requirements to test the applicability of the random cascade model to supersonic turbulence
Doris Folini, Rolf Walder

TL;DR
This paper investigates the applicability of a widely used turbulence model to supersonic regimes, analyzing the accuracy needed in velocity statistics to reliably estimate model parameters and assess its validity.
Contribution
It introduces a Monte Carlo approach to determine the precision required in simulation data to validate the turbulence model in highly compressible flows.
Findings
0.1% accuracy in velocity scaling exponents allows reliable parameter estimation
Simulation data with such accuracy is feasible with current computational resources
Failure to fit parameters accurately may indicate the model's inapplicability
Abstract
A model, which is widely used for inertial rang statistics of supersonic turbulence in the context of molecular clouds and star formation, expresses (measurable) relative scaling exponents Z_p of two-point velocity statistics as a function of two parameters, beta and Delta. The model relates them to the dimension D of the most dissipative structures, D=3-Delta/(1-beta). While this description has proved most successful for incompressible turbulence (beta=Delta=2/3, and D=1), its applicability in the highly compressible regime remains debated. For this regime, theoretical arguments suggest D=2 and Delta=2/3, or Delta=1. Best estimates based on 3D periodic box simulations of supersonic isothermal turbulence yield Delta=0.71 and D=1.9, with uncertainty ranges of Delta in [0.67, 0.78] and D in [2.04,1.60]. With these 5-10\% uncertainty ranges just marginally including the theoretical values…
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