A theory for the emergence of coherent structures in beta-plane turbulence
Nikolaos A. Bakas, Petros J. Ioannou

TL;DR
This paper develops a statistical theory to explain how large-scale coherent structures like jets and vortices emerge in planetary turbulence modeled on a beta-plane, linking bifurcation analysis with numerical simulations.
Contribution
It introduces the Stochastic Structural Stability Theory (S3T) for analyzing the emergence of coherent structures in beta-plane turbulence, providing analytic and numerical insights.
Findings
Analytic expressions for emergent structures are derived.
S3T predicts bifurcation points for structure formation.
Numerical simulations confirm theoretical predictions.
Abstract
Planetary turbulent flows are observed to self-organize into large scale structures such as zonal jets and coherent vortices. One of the simplest models of planetary turbulence is obtained by considering a barotropic flow on a beta-plane channel with turbulence sustained by random stirring. Non-linear integrations of this model show that as the energy input rate of the forcing is increased, the homogeneity of the flow is broken with the emergence of non-zonal, coherent, westward propagating structures and at larger energy input rates by the emergence of zonal jets. We study the emergence of non-zonal coherent structures using a non-equilibrium statistical theory, Stochastic Structural Stability Theory (S3T, previously referred to as SSST). S3T directly models a second order approximation to the statistical mean turbulent state and allows identification of statistical turbulent…
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