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The Ekman Layer is the layer in a fluid where the flow is the result of a balance between pressure gradient, Coriolis and turbulent drag forces. In the picture above, the wind blowing North creates a surface stress and a resulting Ekman spiral is found below it in the column of water.

The Ekman Layer is the layer in a fluid where there is a force balance between pressure gradient force, Coriolis force and turbulent drag. It was first described by Vagn Walfrid Ekman.



Ekman developed the theory of the Ekman layer after Fridtjof Nansen observed that ice drifts at an angle of 20°-40° to the right of the prevailing wind direction while on an Arctic expedition aboard the Fram. Nansen asked his colleague, Vilhelm Bjerknes to set one of his students upon study of the problem. Bjerknes tapped Ekman, who presented his results in 1902 as his doctoral thesis.[1]

Mathematical Formulation

The mathematical formulation of the Ekman layer can be found by assuming a neutrally stratified fluid, with horizontal momentum in balance between the forces of pressure gradient, Coriolis and turbulent drag.

\ -fv = -\frac{1}{\rho_o} \frac{\part p}{\part x}+K_m \frac{\part^2 u}{\part z^2}

\ fu = -\frac{1}{\rho_o} \frac{\part p}{\part y}+K_m \frac{\part^2 v}{\part z^2}

\ 0 = -\frac{1}{\rho_o} \frac{\part p}{\part z},

where \ K_m is the diffusive eddy viscosity, which can be derived using mixing length theory.


Boundary Conditions

There are many regions where an Ekman layer is theoretically plausible; they include the bottom of the atmosphere, near the surface of the earth and ocean, the bottom of the ocean, near the sea floor and at the top of the ocean, near the air-sky interface.

Each of the different regions will have different boundary conditions. We will consider boundary conditions of the Ekman layer in the upper ocean[2]:

at \ z = 0 : A \frac{\part u}{\part z} = \tau^x; A \frac{\part v}{\part z} = \tau^y

where \ \tau is the surface stress of the wind field or ice layer at the top of the ocean.

at \ z \to \infty : u = u_g, v = v_g ,

where \ u_g and \ v_g are the geostrophic flows.


These differential equations can be solved to find:

\ u = u_g + \frac{\sqrt{2}}{fd}e^{z/d}\left [\tau^x cos(z/d - \pi/4) - \tau^y sin(z/d - \pi/4)\right ]

\ v = v_g + \frac{\sqrt{2}}{fd}e^{z/d}\left [\tau^x sin(z/d - \pi/4) + \tau^y cos(z/d - \pi/4)\right ].

and by applying the continuity equation we can have the vertical velocity as following

\ w = \frac{1}{f\rho_o}\left [-\left (\frac{\partial \tau^x}{\partial x} + \frac{\partial \tau^y}{\partial y} \right )e^{z/d}sin(z/d) + \left (\frac{\partial \tau^y}{\partial x} - \frac{\partial \tau^x}{\partial y} \right )(1-e^{z/d}cos(z/d))\right ]

Note that when vertically integrated the volume transport associated with the Ekman spiral is to the right of the wind direction in the Northern Hemisphere.

Experimental Observations of the Ekman Layer

There is much difficulty associated with observing the Ekman layer for two main reasons: the theory is too simplistic as it assumes a constant eddy viscosity, which Ekman himself anticipated[3], saying

It is obvious that \ \left[\nu \right] cannot generally be regarded as a constant when the density of water is not uniform within the region considered

and because it is difficult to design instruments with great enough sensitivity to observe the velocity profile in the ocean.

In the Atmosphere

In the atmosphere, the Ekman solution generally overstates the magnitude of the horizontal wind field because it does not account for the velocity shear in the surface layer. Splitting the boundary layer into the surface layer and the Ekman layer generally yields more accurate results.[4]

In the Ocean

The Ekman layer, with its distinguishing feature the Ekman spiral, is rarely observed in the ocean. The Ekman layer near the surface of the ocean extends only about 10 - 20 meters deep,[4] and instrumentation sensitive enough to observe a velocity profile in such a shallow depth has only been available since around 1980.[2]


Observations of the Ekman layer have only been possible since the development of robust surface moorings and sensitive current meters. Ekman himself developed a current meter to observe the spiral that bears his name, but was not successful.[5] The Vector Measuring Current Meter [6] and the Acoustic Doppler Current Profiler are both used to measure current.


The first observation of the Ekman spiral came in 1980 during the Mixed Layer Experiment.[7]


Ekman transport


  1. ^ [|Cushman-Roisin, Benoit] (1994). "Chapter 5 - The Ekman Layer". Introduction to Geophysical Fluid Dynamics (1st ed.). Prentice Hall. pp. 76–77.  
  2. ^ a b [|Vallis, Geoffrey K.] (2006). "Chapter 2 - Effects of Rotation and Stratification". Atmospheric and Oceanic Fluid Dynamics (1st ed.). Cambridge, UK: Cambridge University Press. pp. 112–113.  
  3. ^ Ekman, V.W. (1905). "On the influence of the earth's rotation on ocean currents". Ark. Mat. Astron. Fys. 2 (11): 1–52.  
  4. ^ a b [|Holton, James R.] (2004). "Chapter 5 - The Planetary Boundary Layer". Dynamic Meteorology. International Geophysics Series. 88 (4th ed.). Burlington, MA: Elsevier Academic Press. pp. 129–130.  
  5. ^ Rudnick, Daniel (2003). "Observations of Momentum Transfer in the Upper Ocean: Did Ekman Get It Right?". Near-Boundary Processes and their Parameterization (Manoa, Hawaii: School of Ocean and Earth Science and Technology).  
  6. ^ Weller, R.A.; Davis, R.E. (1980). "A vector-measuring current meter". Deep-Sea Res. 27: 565–582.  
  7. ^ Davis, R.E.; R. de Szoeke, and P. Niiler. (1981). "Part II: Modelling the mixed layer response". Deep-Sea Res. 28: 1453–1475.  


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