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David Marshall

Professor of Physical Oceanography

Research theme

  • Climate physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Physical oceanography
David.Marshall@physics.ox.ac.uk
Telephone: 01865 (2)72099
Robert Hooke Building, room F47
my personal webpage (external)
  • About
  • Publications

Implications of eddy cancellation on nutrient distribution within subtropical gyres

Journal of Geophysical Research: Oceans John Wiley and Sons, Inc. 123:9 (2018) 6720-6735

Authors:

Edward Doddridge, David Marshall

Abstract:

The role of mesoscale eddies within the nutrient budget of subtropical gyres remains poorly understood and poorly constrained. We explore a new mechanism by which mesoscale eddies may contribute to these nutrient budgets, namely eddy cancellation. Eddy cancellation describes the rectified effect of mesoscale eddies acting to oppose the Eulerian‐mean Ekman pumping. We present an idealized axisymmetric two‐layer model of a nutrient in a wind‐driven gyre and explore the sensitivity of this model to variations in its parameter values. We find that the residual Ekman pumping velocity has a substantial impact on nutrient concentration, as does mode water thickness. These results suggest the response to both residual Ekman pumping and mode water thickness is non‐monotonic: for small values of these parameters the nutrient concentration decreases as the parameter increases. However, beyond a critical value, further increases in Ekman pumping or mode water thickness increase nutrient concentration throughout our highly idealized model. A thin mode water layer promotes vertical diffusion of nutrients from the abyss, while a thicker mode water layer increases productivity by reducing the parametrized particulate flux through the thermocline. The impact of mode water thickness is modulated by the residual Ekman pumping velocity: strong Ekman pumping suppresses the influence of mode water thickness on nutrient concentrations. We use satellite and in‐situ measurements to assess the influence of mode water thickness on primary productivity, and find a statistically significant relationship; thicker mode water correlates with higher productivity. This result is consistent with a small residual Ekman pumping velocity.
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Eddy-mixing entropy and its maximization in forced-dissipative geostrophic turbulence

Journal of Statistical Mechanics: Theory and Experiment IOP Publishing 2018:2018 (2018) 073206

Authors:

Tomos David, Laure Zanna, David Marshall

Abstract:

An equilibrium, or maximum entropy, statistical mechanics theory can be derived for ideal, unforced and inviscid, geophysical flows. However, for all geophysical flows which occur in nature,forcing and dissipation play a major role. Here, a study of eddy-mixing entropy in a forced dissipative barotropic ocean model is presented. We heuristically investigate the temporal evolution of eddy-mixing entropy, as defined for the equilibrium theory, in a strongly forced and dissipative system. It is shown that the eddy-mixing entropy provides a descriptive tool for understanding three stages of the turbulence life cycle: growth of instability; formation of large scale structures; and steady state fluctuations. The fact that the eddy-mixing entropy behaves in a dynamically balanced way is not a priori clear and provides a novel means of quantifying turbulent disorder in geophysical flows. Further, by determining the relationship between the time evolution of entropy and the maximum entropy principle, evidence is found for the action of this principle in a forced dissipative flow. The maximum entropy potential vorticity statistics are calculated for the flow and are compared with numerical simulations. Deficiencies of the maximum entropy statistics are discussed in the context of the mean-field approximation for energy. This study highlights the importance of entropy and statistical mechanics in the study of geostrophic turbulence.
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Atlantic-Pacific asymmetry in deep-water formation

Annual Review of Earth and Planetary Sciences Annual Reviews 46 (2018) 327-352

Authors:

D Ferreira, P Cessi, HK Coxall, A de Boer, HA Dijkstra, SS Drijfhout, T Eldevik, N Harnik, JF McManus, David Marshall, J Nilsson, F Roquet, T Schneider, RC Wills

Abstract:

While the Atlantic Ocean is ventilated by high-latitude deep water formation and exhibits a pole-to-pole overturning circulation, the Pacific Ocean does not. This asymmetric global overturning pattern has persisted for the past 2–3 million years, with evidence for different ventilation modes in the deeper past. In the current climate, the Atlantic-Pacific asymmetry occurs because the Atlantic is more saline, enabling deep convection. To what extent the salinity contrast between the two basins is dominated by atmospheric processes (larger net evaporation over the Atlantic) or oceanic processes (salinity transport into the Atlantic) remains an outstanding question. Numerical simulations have provided support for both mechanisms; observations of the present climate support a strong role for atmospheric processes as well as some modulation by oceanic processes. A major avenue for future work is the quantification of the various processes at play to identify which mechanisms are primary in different climate states.
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A Model of the Ocean Overturning Circulation with Two Closed Basins and a Reentrant Channel

JOURNAL OF PHYSICAL OCEANOGRAPHY 47:12 (2017) 2887-2906

Authors:

R Ferrari, L-P Nadeau, DP Marshall, LC Allison, HL Johnson
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Submesoscale Instabilities in Mesoscale Eddies

JOURNAL OF PHYSICAL OCEANOGRAPHY 47:12 (2017) 3061-3085

Authors:

L Brannigan, DP Marshall, ACN Garabato, AJG Nurser, J Kaiser
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