The Estuarine Circulation
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W. Rockwell Geyer [1] ; Parker MacCready [2]
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[1] Woods Hole Oceanographic Institution
Woods Hole Oceanographic Institution
Town of Falmouth, Estados Unidos
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[2] University of Washington
University of Washington
Estados Unidos
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- Localización: Annual review of fluid mechanics, ISSN 0066-4189, Nº. 46, 2014, págs. 175-197
- Idioma: inglés
- Texto completo no disponible (Saber más ...)
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Resumen
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.
