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The Estuarine Circulation

2013/08/29 by W. Rockwell Geyer, Parker MacCready · 6 citations
Earth and Planetary Sciences · Environmental Science · #Oceanographic and Atmospheric Processes #Tropical and Extratropical Cyclones Research #Coastal wetland ecosystem dynamics

paper · pdf · doi:10.1146/annurev-fluid-010313-141302

Abstract

Recent research in estuaries challenges the long-standing paradigm of the gravitationally driven estuarine circulation. In estuaries with relatively strong tidal forcing and modest buoyancy forcing, the tidal variation in stratification leads to a tidal straining circulation driven by tidal variation in vertical mixing, with a magnitude that may significantly exceed the gravitational circulation. For weakly stratified estuaries, vertical and lateral advection are also important contributors to the tidally driven residual circulation. The apparent contradiction with the conventional paradigm is resolved when the estuarine parameter space is mapped with respect to a mixing parameter M that is based on the ratio of the tidal timescale to the vertical mixing timescale. Estuaries with high M values exhibit strong tidal nonlinearity, and those with small M values show conventional estuarine dynamics. Estuaries with intermediate mixing rates show marked transitions between these regimes at timescales of the spring-neap cycle.

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