Scalar mixing in non-Markovian homogeneous isotropic synthetic turbulence
Pratyush S. Awasthi, Joaquim P. Jossy, Amitabh Bhattacharya, Prateek Gupta

TL;DR
This paper demonstrates that non-Markovian velocity fields are crucial for accurately modeling turbulent mixing, showing that synthetic non-Markovian fields better replicate DNS results than Markovian ones.
Contribution
The study introduces a synthetic turbulence model incorporating non-Markovian velocity fields with scale-dependent decorrelation times, improving the representation of mixing dynamics.
Findings
Non-Markovian synthetic fields match DNS scalar spectra at low Schmidt numbers.
Markovian fields underpredict scalar variance production and dissipation.
Non-Markovianity is essential for realistic turbulent mixing simulations.
Abstract
We show that non-Markovianity of the velocity field is an essential property of turbulent mixing. We demonstrate this via passive scalar mixing by synthetically generated stochastic velocity fields. Including a separate velocity decorrelation time scale for each spatial scale (random sweeping) yields an essentially non-Markovian velocity field with a finite time memory decaying as -5 (for a decaying spectrum) instead of an exponential decay (Markovian), which is obtained by including a constant time scale for all spatial scales, irrespective of the filtering function. We characterize the Lagrangian mixing statistics of both the Markovian and non-Markovian synthetic fields and compare them against a corresponding incompressible direct numerical simulation (DNS). We also study diffusive passive scalar mixing in the Schmidt number range Sc<1 using the DNS and the synthetic fields. While…
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Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Combustion and flame dynamics · Laser-Plasma Interactions and Diagnostics
