Evolution of some Fluid Dynamical Paradigms about the Oceanic General Circulation

J.C. McWilliams

Institute of Geophysics and Planetary Physics
UCLA

Abstract-
The field measurements recently ended for the World Ocean Circulation Experiment (WOCE). This was an enormous undertaking involving many satellites, many tens of ships, and many hundreds of autonomous platforms overseen by hundreds of scientists from many nations over a period of nearly two decades. While physical oceanographers took pride in these conspicuous expenditures of effort and funds, they now struggle with the resulting data abundance---albeit still with significant sampling sparsity for many relevant features---in order to distill the essential lessons about the controlling processes and dynamical balances for the general circulation. It is thus timely to summarize for a broader community of fluid dynamicists what these essential lessons are. The discussion will be set in the context of historically prevailing ideas about oceanic circulation dynamics to consider how these evolved during the WOCE era. The following topics will be addressed: * Horizontal Mass Transport: Adjustments to Wind-Driven Sverdrup Balance * Pycnocline Circulation: Planetary Geostrophy and Subduction * Abyssal Thermohaline Circulation: Connecting the Vertical Motions in Stommel-Arons Balance * Surface Circulation: Mixed and Ekman Layers, Surface-Wave Effects, and Climate Feedbacks * Mesoscale Eddies: Quasi-Adiabatic Mixing and Lagrangian-Mean Advection * Diapycnal Microscale Mixing: Topographic Enhancements of Breaking Internal Waves * Overflows: Renewal of Abyssal Water Masses by Entraining Gravity Currents


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