A rotating flow about a specified axis has a uθ=rΩu_\theta=r\Omega. It may also have radial and axial components. The angular velocity Ω\Omega describes its local rotation rate around that axis.

Rigid rotation

The velocity u=(Ω0x2,Ω0x1,0)u=(-\Omega_0 x_2,\Omega_0 x_1,0), with constant Ω0\Omega_0, is rigid rotation. It is divergence free, has zero rate of strain, and satisfies both unforced Euler and Navier–Stokes equations with

p=12Ω02(x12+x22),p=\tfrac12\Omega_0^2(x_1^2+x_2^2),

since the Laplacian of this linear velocity is zero. On the whole space it has infinite kinetic energy.

Differential rotation

For an axisymmetric field, variation of Ω(r,z)\Omega(r,z) with position is differential rotation. Its radial shear contribution satisfies

2D(u)rθ=ruθuθr=rrΩ.2D(u)_{r\theta}=\partial_r u_\theta-\frac{u_\theta}{r} =r\partial_r\Omega.

Consequently a nonzero azimuthal velocity does not by itself imply nonzero shear.