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Stokes drift

From Wikipedia, the free encyclopedia
Average velocity of a fluid parcel in a gravity wave
Stokes drift in deepwater waves, with awave length of about twice the water depth.
Stokes drift in shallow water waves, with a wave length much longer than the water depth.
The red circles are the present positions of massless particles, moving with theflow velocity. The light-blue line gives thepath of these particles, and the light-blue circles the particle position after eachwave period. The white dots are fluid particles, also followed in time. In the cases shown here, themean Eulerian horizontal velocity below the wavetrough is zero.
Observe that thewave period, experienced by a fluid particle near thefree surface, is different from thewave period at a fixed horizontal position (as indicated by the light-blue circles). This is due to theDoppler shift.
An expanse ofdriftwood along the northerncoast ofWashington state. Stokes drift – besides e.g.Ekman drift andgeostrophic currents – is one of the relevant processes in the transport ofmarine debris.[1]

For a purewavemotion influid dynamics, theStokes drift velocity is theaveragevelocity when following a specificfluid parcel as it travels with thefluid flow. For instance, a particle floating at thefree surface ofwater waves, experiences a net Stokes drift velocity in the direction ofwave propagation.

More generally, the Stokes drift velocity is the difference between theaverageLagrangianflow velocity of a fluid parcel, and the averageEulerianflow velocity of thefluid at a fixed position. Thisnonlinear phenomenon is named afterGeorge Gabriel Stokes, who derived expressions for this drift inhis 1847 study ofwater waves.

TheStokes drift is the difference in end positions, after a predefined amount of time (usually onewave period), as derived from a description in theLagrangian and Eulerian coordinates. The end position in theLagrangian description is obtained by following a specific fluid parcel during the time interval. The corresponding end position in theEulerian description is obtained by integrating theflow velocity at a fixed position—equal to the initial position in the Lagrangian description—during the same time interval.

The Stokes drift velocity equals the Stokes drift divided by the considered time interval.Often, the Stokes drift velocity is loosely referred to as Stokes drift.Stokes drift may occur in all instances of oscillatory flow which areinhomogeneous in space. For instance inwater waves,tides andatmospheric waves.

In theLagrangian description, fluid parcels may drift far from their initial positions. As a result, the unambiguous definition of anaverage Lagrangian velocity and Stokes drift velocity, which can be attributed to a certain fixed position, is by no means a trivial task. However, such an unambiguous description is provided by theGeneralized Lagrangian Mean (GLM) theory ofAndrews and McIntyre in 1978.[2]

The Stokes drift is important for themass transfer of various kinds of material and organisms by oscillatory flows. It plays a crucial role in the generation ofLangmuir circulations.[3]For nonlinear andperiodic water waves, accurate results on the Stokes drift have been computed and tabulated.[4]

Mathematical description

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TheLagrangian motion of a fluid parcel withposition vectorx =ξ(α, t) in the Eulerian coordinates is given by[5]

ξ˙=ξt=u(ξ(α,t),t),{\displaystyle {\dot {\boldsymbol {\xi }}}={\frac {\partial {\boldsymbol {\xi }}}{\partial t}}=\mathbf {u} {\big (}{\boldsymbol {\xi }}({\boldsymbol {\alpha }},t),t{\big )},}

where

ξ/∂t is thepartial derivative ofξ(α,t) with respect tot,
ξ(α,t) is the Lagrangian position vector of a fluid parcel,
u(x,t) is the Eulerianvelocity,
x is the position vector in theEulerian coordinate system,
α is the position vector in theLagrangian coordinate system,
t istime.

Often, the Lagrangian coordinatesα are chosen to coincide with the Eulerian coordinatesx at the initial timet =t0:[5]

ξ(α,t0)=α.{\displaystyle {\boldsymbol {\xi }}({\boldsymbol {\alpha }},t_{0})={\boldsymbol {\alpha }}.}

If theaverage value of a quantity is denoted by an overbar, then the average Eulerian velocity vectorūE and average Lagrangian velocity vectorūL are

u¯E=u(x,t)¯,u¯L=ξ˙(α,t)¯=(ξ(α,t)t)¯=u(ξ(α,t),t)¯.{\displaystyle {\begin{aligned}{\bar {\mathbf {u} }}_{\text{E}}&={\overline {\mathbf {u} (\mathbf {x} ,t)}},\\{\bar {\mathbf {u} }}_{\text{L}}&={\overline {{\dot {\boldsymbol {\xi }}}({\boldsymbol {\alpha }},t)}}={\overline {\left({\frac {\partial {\boldsymbol {\xi }}({\boldsymbol {\alpha }},t)}{\partial t}}\right)}}={\overline {{\boldsymbol {u}}{\big (}{\boldsymbol {\xi }}({\boldsymbol {\alpha }},t),t{\big )}}}.\end{aligned}}}

Different definitions of theaverage may be used, depending on the subject of study (seeergodic theory):

The Stokes drift velocityūS is defined as the difference between the average Eulerian velocity and the average Lagrangian velocity:[6]

u¯S=u¯Lu¯E.{\displaystyle {\bar {\mathbf {u} }}_{\text{S}}={\bar {\mathbf {u} }}_{\text{L}}-{\bar {\mathbf {u} }}_{\text{E}}.}

In many situations, themapping of average quantities from some Eulerian positionx to a corresponding Lagrangian positionα forms a problem. Since a fluid parcel with labelα traverses along apath of many different Eulerian positionsx, it is not possible to assignα to a uniquex.A mathematically sound basis for an unambiguous mapping between average Lagrangian and Eulerian quantities is provided by the theory of thegeneralized Lagrangian mean (GLM) byAndrews and McIntyre (1978).

Example: A one-dimensional compressible flow

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For the Eulerian velocity as a monochromatic wave of any nature in a continuous medium:u=u^sin(kxωt),{\displaystyle u={\hat {u}}\sin(kx-\omega t),} one readily obtains by theperturbation theory – withku^/ω{\displaystyle k{\hat {u}}/\omega } as a small parameter – for the particle positionx=ξ(ξ0,t){\displaystyle x=\xi (\xi _{0},t)}:

ξ˙=u(ξ,t)=u^sin(kξωt),{\displaystyle {\dot {\xi }}=u(\xi ,t)={\hat {u}}\sin(k\xi -\omega t),}
ξ(ξ0,t)ξ0+u^ωcos(kξ0ωt)14ku^2ω2sin2(kξ0ωt)+12ku^2ωt.{\displaystyle \xi (\xi _{0},t)\approx \xi _{0}+{\frac {\hat {u}}{\omega }}\cos(k\xi _{0}-\omega t)-{\frac {1}{4}}{\frac {k{\hat {u}}^{2}}{\omega ^{2}}}\sin 2(k\xi _{0}-\omega t)+{\frac {1}{2}}{\frac {k{\hat {u}}^{2}}{\omega }}t.}

Here the last term describes the Stokes drift velocity12ku^2/ω.{\displaystyle {\tfrac {1}{2}}k{\hat {u}}^{2}/\omega .}[7]

Example: Deep water waves

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Stokes drift under periodic waves in deep water, for aperiodT = 5 s and a mean water depth of 25 m.Left: instantaneous horizontalflow velocities.Right:average flow velocities. Black solid line: average Eulerian velocity; red dashed line: average Lagrangian velocity, as derived from theGeneralized Lagrangian Mean (GLM).
See also:Airy wave theory andStokes wave

The Stokes drift was formulated forwater waves byGeorge Gabriel Stokes in 1847. For simplicity, the case ofinfinitely deep water is considered, withlinearwave propagation of asinusoidal wave on thefree surface of a fluid layer:[8]

η=acos(kxωt),{\displaystyle \eta =a\cos(kx-\omega t),}

where

η is theelevation of thefree surface in thez direction (meters),
a is the waveamplitude (meters),
k is thewave number:k = 2π/λ (radians per meter),
ω is theangular frequency:ω = 2π/T (radians persecond),
x is the horizontalcoordinate and the wave propagation direction (meters),
z is the verticalcoordinate, with the positivez direction pointing out of the fluid layer (meters),
λ is thewave length (meters),
T is thewave period (seconds).

As derived below, the horizontal componentūS(z) of the Stokes drift velocity for deep-water waves is approximately:[9]

u¯Sωka2e2kz=4π2a2λTe4πz/λ.{\displaystyle {\bar {u}}_{\text{S}}\approx \omega ka^{2}{\text{e}}^{2kz}={\frac {4\pi ^{2}a^{2}}{\lambda T}}{\text{e}}^{4\pi z/\lambda }.}

As can be seen, the Stokes drift velocityūS is a nonlinear quantity in terms of the waveamplitudea. Further, the Stokes drift velocity decays exponentially with depth: at a depth of a quarter wavelength,z = −λ/4, it is about 4% of its value at the meanfree surface,z = 0.

Derivation

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It is assumed that the waves are ofinfinitesimalamplitude and thefree surface oscillates around themean levelz = 0. The waves propagate under the action of gravity, with aconstantaccelerationvector bygravity (pointing downward in the negativez direction). Further the fluid is assumed to beinviscid[10] andincompressible, with a constantmass density. The fluidflow isirrotational. At infinite depth, the fluid is taken to be atrest.

Now theflow may be represented by avelocity potentialφ, satisfying theLaplace equation and[8]

φ=ωkaekzsin(kxωt).{\displaystyle \varphi ={\frac {\omega }{k}}a{\text{e}}^{kz}\sin(kx-\omega t).}

In order to havenon-trivial solutions for thiseigenvalue problem, thewave length andwave period may not be chosen arbitrarily, but must satisfy the deep-waterdispersion relation:[11]

ω2=gk{\displaystyle \omega ^{2}=gk}

withg theacceleration bygravity in (m/s2). Within the framework oflinear theory, the horizontal and vertical components,ξx andξz respectively, of the Lagrangian positionξ are[9]

ξx=x+φxdt=xaekzsin(kxωt),ξz=z+φzdt=z+aekzcos(kxωt).{\displaystyle {\begin{aligned}\xi _{x}&=x+\int {\frac {\partial \varphi }{\partial x}}\,{\text{d}}t=x-a{\text{e}}^{kz}\sin(kx-\omega t),\\\xi _{z}&=z+\int {\frac {\partial \varphi }{\partial z}}\,{\text{d}}t=z+a{\text{e}}^{kz}\cos(kx-\omega t).\end{aligned}}}

The horizontal componentūS of the Stokes drift velocity is estimated by using aTaylor expansion aroundx of the Eulerian horizontal velocity componentux = ∂ξx / ∂t at the positionξ:[5]

u¯S=ux(ξ,t)¯ux(x,t)¯=[ux(x,t)+(ξxx)ux(x,t)x+(ξzz)ux(x,t)z+]¯ux(x,t)¯(ξxx)2ξxxt¯+(ξzz)2ξxzt¯=[aekzsin(kxωt)][ωkaekzsin(kxωt)]¯+[aekzcos(kxωt)][ωkaekzcos(kxωt)]¯=ωka2e2kz[sin2(kxωt)+cos2(kxωt)]¯=ωka2e2kz.{\displaystyle {\begin{aligned}{\bar {u}}_{\text{S}}&={\overline {u_{x}({\boldsymbol {\xi }},t)}}-{\overline {u_{x}(\mathbf {x} ,t)}}\\&={\overline {\left[u_{x}(\mathbf {x} ,t)+(\xi _{x}-x){\frac {\partial u_{x}(\mathbf {x} ,t)}{\partial x}}+(\xi _{z}-z){\frac {\partial u_{x}(\mathbf {x} ,t)}{\partial z}}+\cdots \right]}}-{\overline {u_{x}(\mathbf {x} ,t)}}\\&\approx {\overline {(\xi _{x}-x){\frac {\partial ^{2}\xi _{x}}{\partial x\,\partial t}}}}+{\overline {(\xi _{z}-z){\frac {\partial ^{2}\xi _{x}}{\partial z\,\partial t}}}}\\&={\overline {\left[-a{\text{e}}^{kz}\sin(kx-\omega t)\right]\left[-\omega ka{\text{e}}^{kz}\sin(kx-\omega t)\right]}}\\&+{\overline {\left[a{\text{e}}^{kz}\cos(kx-\omega t)\right]\left[\omega ka{\text{e}}^{kz}\cos(kx-\omega t)\right]}}\\&={\overline {\omega ka^{2}{\text{e}}^{2kz}\left[\sin ^{2}(kx-\omega t)+\cos ^{2}(kx-\omega t)\right]}}\\&=\omega ka^{2}{\text{e}}^{2kz}.\end{aligned}}}

See also

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References

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Historical

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Other

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Notes

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  1. ^SeeKubota (1994).
  2. ^SeeCraik (1985), page 105–113.
  3. ^Seee.g.Craik (1985), page 120.
  4. ^Solutions of the particle trajectories in fully nonlinear periodic waves and the Lagrangian wave period they experience can for instance be found in:
    J.M. Williams (1981). "Limiting gravity waves in water of finite depth".Philosophical Transactions of the Royal Society A.302 (1466):139–188.Bibcode:1981RSPTA.302..139W.doi:10.1098/rsta.1981.0159.S2CID 122673867.
    J.M. Williams (1985).Tables of progressive gravity waves. Pitman.ISBN 978-0-273-08733-5.
  5. ^abcSeePhillips (1977), page 43.
  6. ^See e.g.Craik (1985), page 84.
  7. ^SeeFalkovich (2011), pages 71–72. There is a typo in the coefficient of the superharmonic term in Eq. (2.20) on page 71, i.e14{\displaystyle -{\tfrac {1}{4}}} instead of+12.{\displaystyle +{\tfrac {1}{2}}.}
  8. ^abSee e.g.Phillips (1977), page 37.
  9. ^abSeePhillips (1977), page 44. OrCraik (1985), page 110.
  10. ^Viscosity has a pronounced effect on the mean Eulerian velocity and mean Lagrangian (or mass transport) velocity, but much less on their difference: the Stokes drift outside theboundary layers near bed and free surface, see for instanceLonguet-Higgins (1953). OrPhillips (1977), pages 53–58.
  11. ^Seee.g.Phillips (1977), page 38.
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