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Velocity distribution in a Rankine vortex.
Animation of a Rankine vortex. Free-floating test particles reveal the velocity and vorticity pattern.

The Rankine vortex is a simple mathematical model of a vortex in a viscous fluid. It is named after its discoverer, William John Macquorn Rankine.

The vortices observed in nature are usually modelled with an irrotational (potential or free) vortex. However, in a potential vortex, the velocity becomes infinite at the vortex center. In reality, very close to the origin, the motion resembles a solid body rotation. The Rankine vortex model assumes a solid-body rotation inside a cylinder of radius a and a potential vortex outside the cylinder. The radius a is referred to as the vortex-core radius. The velocity components (vr,vθ,vz) of the Rankine vortex, expressed in terms of the cylindrical-coordinate system (r,θ,z) are given by[1]

vr=0,vθ(r)=Γ2π{r/a2ra,1/rr>a,vz=0

where Γ is the circulation strength of the Rankine vortex. Since solid-body rotation is characterized by an azimuthal velocity Ωr, where Ω is the constant angular velocity, one can also use the parameter Ω=Γ/(2πa2) to characterize the vortex.

The vorticity field (ωr,ωθ,ωz) associated with the Rankine vortex is

ωr=0,ωθ=0,ωz={2Ωra,0r>a.

At all points inside the core of the Rankine vortex, the vorticity is uniform at twice the angular velocity of the core; whereas vorticity is zero at all points outside the core because the flow there is irrotational.

In reality, vortex cores are not always circular; and vorticity is not exactly uniform throughout the vortex core.

See also

References

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