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Circulation (physics)

Line integral of the fluid velocity around a closed curve

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The term circulation was introduced by William Thomson (later Lord Kelvin) in 1869 to denote the line integral of velocity around a closed curve as a kinematic measure of rotational motion in a fluid, independent of any particular application. In aerodynamics, circulation appears in a more specialised context in relation to the calculation of lift, where it is evaluated on contours enclosing a body under additional flow assumptions. In this context, circulation was first used independently by Frederick Lanchester, Ludwig Prandtl, Martin Kutta and Nikolay Zhukovsky. It is usually denoted by Γ (uppercase gamma).

Definition and properties

If V is a vector field and dl is a vector representing the differential length of a small element of a defined curve, the contribution of that differential length to circulation is dΓ: dΓ=V⋅dl=|V||dl|cos⁡θ.

Here, θ is the angle between the vectors V and dl.

The circulation Γ of a vector field V around a closed curve C is the line integral: Γ=∮CV⋅dl.

In a conservative vector field this integral evaluates to zero for every closed curve. That means that a line integral between any two points in the field is independent of the path taken. It also implies that the vector field can be expressed as the gradient of a scalar function, which is called a potential.

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