A hierarchy of energy- and flux-budget (EFB) turbulence closure models for stably stratified geophysical flows
S.S. Zilitinkevich (1-4), T. Elperin (5), N. Kleeorin (5), I., Rogachevskii (5), I. Esau (3) ((1) FMI, (2) Univ. of Helsinki, (3), NERSC/BCCR, (4) Univ. Nizhniy Novgorod, (5) Ben-Gurion Univ.)

TL;DR
This paper develops a hierarchical set of turbulence closure models for stratified geophysical flows, incorporating physical principles, Earth rotation, and different turbulence regimes, from steady-state to non-local models.
Contribution
It introduces a new hierarchy of EFB turbulence closure models that account for various turbulence regimes and includes a novel relaxation equation for the dissipation time-scale.
Findings
Models distinguish strong and weak turbulence regimes.
Turbulent Prandtl number behavior varies with Ri.
Closure models applicable from boundary layers to the free atmosphere.
Abstract
In this paper we advance physical background of the energy- and flux-budget turbulence closure based on the budget equations for the turbulent kinetic and potential energies and turbulent fluxes of momentum and buoyancy, and a new relaxation equation for the turbulent dissipation time-scale. The closure is designed for stratified geophysical flows from neutral to very stable and accounts for the Earth rotation. In accordance to modern experimental evidence, the closure implies maintaining of turbulence by the velocity shear at any gradient Richardson number Ri, and distinguishes between the two principally different regimes: "strong turbulence" at Ri << 1 typical of boundary-layer flows and characterised by the practically constant turbulent Prandtl number; and "weak turbulence" at Ri > 1 typical of the free atmosphere or deep ocean, where the turbulent Prandtl number asymptotically…
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