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Published April 2006 | Published
Journal Article Open

Scaling Baroclinic Eddy Fluxes: Vortices and Energy Balance

Abstract

The eddy heat flux generated by the statistically equilibrated baroclinic instability of a uniform, horizontal temperature gradient is studied using a two-mode f-plane quasigeostrophic model. An overview of the dependence of the eddy diffusivity D on the bottom friction κ, the deformation radius λ, the vertical variation of the large-scale flow U, and the domain size L is provided by numerical simulations at 70 different values of the two nondimensional control parameters κλ/U and L/λ. Strong, axisymmetric, well-separated baroclinic vortices dominate both the barotropic vorticity and the temperature fields. The core radius of a single vortex is significantly larger than λ but smaller than the eddy mixing length ℓ_mix. On the other hand, the typical vortex separation is comparable to ℓ_mix. Anticyclonic vortices are hot, and cyclonic vortices are cold. The motion of a single vortex is due to barotropic advection by other distant vortices, and the eddy heat flux is due to the systematic migration of hot anticyclones northward and cold cyclones southward. These features can be explained by scaling arguments and an analysis of the statistically steady energy balance. These arguments result in a relation between D and ℓ_mix. Earlier scaling theories based on coupled Kolmogorovian cascades do not account for these coherent structures and are shown to be unreliable. All of the major properties of this dilute vortex gas are exponentially sensitive to the strength of the bottom drag. As the bottom drag decreases, both the vortex cores and the vortex separation become larger. Provided that ℓ_mix remains significantly smaller than the domain size, then local mixing length arguments are applicable, and our main empirical result is ℓ_mix ≈ 4λ exp(0.3U/κλ).

Additional Information

© 2006 American Meteorological Society. Received: April 26, 2005; Accepted: September 19, 2005. We thank Lien Hua and Patrice Klein for providing the spectral code used in this work. We have benefited from conversations with Paola Cessi, Stefan Llewellyn Smith, Rick Salmon, and Geoff Vallis. Comments from K. Shafer Smith and an anonymous reviewer significantly improved the presentation This work was supported by the National Science Foundation under the Collaborations in Mathematical Geo sciences initiative (Grants ATM0222109 and ATM0222104). AFT also gratefully acknowledges the support of an NDSEG Fellowship.

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