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Hierarchical parcel-swapping representation of turbulent mixing. Part 4. Extension to the viscous range and to mixing of scalars with non-unity Schmidt numbers

Published online by Cambridge University Press:  30 September 2025

Masoomeh Behrang
Affiliation:
330 EB, Brigham Young University, Provo, UT 84602, USA
Tommy Starick
Affiliation:
Brandenburg University of Technology Cottbus-Senftenberg, Cottbus, Germany
Isaac Wheeler
Affiliation:
330 EB, Brigham Young University, Provo, UT 84602, USA
Heiko Schmidt
Affiliation:
Brandenburg University of Technology Cottbus-Senftenberg, Cottbus, Germany
Alan Kerstein
Affiliation:
Consultant, 72 Lomitas Road, Danville, CA 94526, USA
David Lignell*
Affiliation:
330 EB, Brigham Young University, Provo, UT 84602, USA
*
Corresponding author: David Lignell, davidlignell@byu.edu

Abstract

Hierarchical parcel swapping (HiPS) is a multiscale stochastic model of turbulent mixing based on a binary tree. Length scales decrease geometrically with increasing tree level, and corresponding time scales follow inertial range scaling. Turbulent eddies are represented by swapping subtrees. Lowest-level swaps change fluid parcel pairings, with new pairings instantly mixed. This formulation suitable for unity Schmidt number $Sc$ is extended to non-unity $Sc$. For high $Sc$, the tree is extended to the Batchelor level, assigning the same time scale (governing the rate of swap occurrences) to the added levels as the time scale at the base of the $Sc=3$ tree. For low $Sc$, a swap at the Obukhov–Corrsin level mixes all parcels within corresponding subtrees. Well-defined model analogues of turbulent diffusivity, and mean scalar-variance production and dissipation rates are identified. Simulations idealising stationary homogeneous turbulence with an imposed scalar gradient reproduce various statistical properties of viscous-range and inertial-range pair dispersion, and of the scalar power spectrum in the inertial-advective, inertial-diffusive and viscous-advective regimes. The viscous-range probability density functions of pair separation and scalar dissipation agree with applicable theory, including the stretched-exponential tail shape associated with viscous-range scalar intermittency. Previous observation of that tail shape for $Sc=1$, heretofore not modelled or explained, is reproduced. Comparisons to direct numerical simulation allow evaluation of empirical coefficients, facilitating quantitative applications. Parcel-pair mixing is a common mixing treatment, e.g. in subgrid closures for coarse-grained flow simulation, so HiPS can improve model physics simply by smarter (yet nearly cost-free) selection of pairs to be mixed.

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Type
JFM Papers
Copyright
© The Author(s), 2025. Published by Cambridge University Press

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