Journal article
Mixing and dissipation in a geostrophic buoyancy-driven circulation
CA Vreugdenhil, B Gayen, RW Griffiths
Journal of Geophysical Research Oceans | AMER GEOPHYSICAL UNION | Published : 2016
DOI: 10.1002/2016JC011691
Abstract
Turbulent mixing and energy dissipation have important roles in the global circulation but are not resolved by ocean models. We use direct numerical simulations of a geostrophic circulation, resolving turbulence and convection, to examine the rates of dissipation and mixing. As a starting point, we focus on circulation in a rotating rectangular basin forced by a surface temperature difference but no wind stress. Emphasis is on the geostrophic regime for the horizontal circulation, but also on the case of strong buoyancy forcing (large Rayleigh number), which implies a turbulent convective boundary layer. The computed results are consistent with existing scaling theory that predicts dynamics ..
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Awarded by Australian Research Council
Funding Acknowledgements
The research was supported by Australian Research Council grant DP140103706 and BG was funded by an Australian Research Council Discovery Early Career Fellowship DE140100089. Numerical computations were carried out on the Australian National Computational Infrastructure, ANU. Model output can be obtained through a written request to the corresponding author (email: Catherine.Vreugdenhil@anu.edu.au). We thank A. McC. Hogg for providing helpful comments and feedback on an earlier version of this paper.