Summary

Geophysical fluid dynamics of zonal flows explores the formation, maintenance and variability of large-scale east–west winds found in planetary atmospheres and oceans. These jets arise from the interplay of earth’s rotation, stratification and turbulent motions, yielding highly anisotropic flows that dominate transport of momentum, heat and tracers. Central to their dynamics is the β-effect, which introduces a latitudinal gradient of planetary vorticity and fosters the organisation of turbulence into alternating zonal bands. Energy injected at small scales by convection or baroclinic instability is redistributed through nonlinear interactions: Reynolds stresses extract energy from eddies to reinforce jets, while an inverse cascade may transfer kinetic energy upscale until arrested by planetary waves. The Rhines scale sets the characteristic jet spacing by balancing eddy advection against Rossby-wave propagation. In oceanic contexts, baroclinic turbulence modulates buoyancy transport and deep stratification; in planetary atmospheres, zonostrophic regimes shape the banded patterns of gas giants and influence global circulation on Earth. Understanding these flows is crucial for improved climate modelling, precise weather forecasting and the interpretation of spacecraft observations of other worlds.

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Geophysical Fluid Dynamics of Zonal Flows publication trend

The graph below shows the total number of articles in geophysical fluid dynamics of zonal flows across all publications each year (not limited to Nature Index journals).

Technical terms

Zonal jets: Predominantly east–west flows organised into alternating bands by rotation and turbulence.

β-effect: Variation of planetary vorticity with latitude that induces anisotropy in turbulent flows.

Rhines scale: Length scale at which turbulent eddy motions are arrested by Rossby-wave propagation, setting jet spacing.

Reynolds stresses: Momentum fluxes arising from correlated velocity fluctuations that transfer energy between eddies and mean flow.

Baroclinic turbulence: Turbulence driven by buoyancy and vertical shear in stratified rotating fluids, critical for meridional transport.

References

  1. Direct driving of simulated planetary jets by upscale energy transfer. Astronomy & Astrophysics (2023).
  2. Vertical Structure of Buoyancy Transport by Ocean Baroclinic Turbulence. Geophysical Research Letters (2023).
  3. Anisotropic turbulence and zonal jets in rotating flows with a β-effect. Nonlinear Processes in Geophysics (2006).
  4. Zonal jets experiments in the gas giants’ zonostrophic regime. Icarus (2023).

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