Gravitational Circulation
Gravitational Circulation is a theoretical construct in estuarine dynamics denoting the residual overturning circulation driven by horizontal density gradients, wherein freshwater inflow at the surface and seawater intrusion at depth are maintained by gravitational adjustment and buoyancy-driven pressure gradients.
81
Publications
5.3K
Citations
206
Authors
98
Institutions
Publications per year
2017–2026
20
81
W. Rockwell Geyer, Parker MacCready · Annual Review of Fluid Mechanics · 2013 · 629 citations · Full text
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Leibniz Institute for Baltic Sea Research Warnemünde, Germany
4 publications · 682 citations
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1–5 of 206
98
University of Washington
Seattle, United States
7 h-index
11 publications
2.4K citations

National Oceanography Centre
Southampton, United Kingdom
4 h-index
14 publications
482 citations

Delft University of Technology
Delft, The Netherlands
3 h-index
4 publications
339 citations
University of Delaware
Newark, United States
3 h-index
4 publications
350 citations
William & Mary
Williamsburg, United States
3 h-index
10 publications
222 citations
University of Maryland Center for Environmental Science
Cambridge, United States
3 h-index
7 publications
394 citations
Woods Hole Oceanographic Institution
Falmouth, United States
3 h-index
3 publications
674 citations
State Key Laboratory of Satellite Ocean Environment Dynamics
Hangzhou, China
3 h-index
6 publications
253 citations
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JGR · 17 publications · 1.1K citations
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8 publications · 1.1K citations
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6 publications · 304 citations
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3 publications · 177 citations
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2 publications · 41 citations
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