Vorticity equation
The vorticity equation of fluid dynamics describes evolution of the vorticity ω of a particle of a fluid as it moves with its flow, that is, the local rotation of the fluid (in terms of vector calculus this is the curl of the flow velocity). The equation is:
Continuum mechanics  

Laws


where D/Dt is the material derivative operator, u is the flow velocity, ρ is the local fluid density, p is the local pressure, τ is the viscous stress tensor and B represents the sum of the external body forces. The first source term on the right hand side represents vortex stretching.
The equation is valid in the absence of any concentrated torques and line forces, for a compressible Newtonian fluid.
In the case of incompressible (i.e. low Mach number) and isotropic fluids, with conservative body forces, the equation simplifies to the vorticity transport equation
where ν is the kinematic viscosity and ∇^{2} is the Laplace operator.
Physical interpretation
 The term Dω/Dt on the lefthand side is the material derivative of the vorticity vector ω. It describes the rate of change of vorticity of the moving fluid particle. This change can be attributed to unsteadiness in the flow (∂ω/∂t, the unsteady term) or due to the motion of the fluid particle as it moves from one point to another ((u ∙ ∇)ω, the convection term).
 The term (ω ∙ ∇) u on the righthand side describes the stretching or tilting of vorticity due to the flow velocity gradients. Note that (ω ∙ ∇) u is a vector quantity, as ω ∙ ∇ is a scalar differential operator, while ∇u is a nineelement tensor quantity.
 The term ω(∇ ∙ u) describes stretching of vorticity due to flow compressibility. It follows from the NavierStokes equation for continuity, namely
 where v = 1/ρ is the specific volume of the fluid element. One can think of ∇ ∙ u as a measure of flow compressibility. Sometimes the negative sign is included in the term.
 The term 1/ρ^{2}∇ρ × ∇p is the baroclinic term. It accounts for the changes in the vorticity due to the intersection of density and pressure surfaces.
 The term ∇ × (∇ ∙ τ/ρ), accounts for the diffusion of vorticity due to the viscous effects.
 The term ∇ × B provides for changes due to external body forces. These are forces that are spread over a threedimensional region of the fluid, such as gravity or electromagnetic forces. (As opposed to forces that act only over a surface (like drag on a wall) or a line (like surface tension around a meniscus).
Simplifications
 In case of conservative body forces, ∇ × B = 0.
 For a barotropic fluid, ∇ρ × ∇p = 0. This is also true for a constant density fluid (including incompressible fluid) where ∇ρ = 0. Note that this is not the same as an incompressible flow, for which the barotropic term cannot be neglected.
 For inviscid fluids, the viscosity tensor τ is zero.
Thus for an inviscid, barotropic fluid with conservative body forces, the vorticity equation simplifies to
Alternately, in case of incompressible, inviscid fluid with conservative body forces,
For a brief review of additional cases and simplifications, see also.[1]
Derivation
The vorticity equation can be derived from the Navier–Stokes equation for the conservation of angular momentum. In the absence of any concentrated torques and line forces, one obtains
Now, vorticity is defined as the curl of the flow velocity vector. Taking the curl of momentum equation yields the desired equation.
The following identities are useful in derivation of the equation:
where ϕ is any scalar field.
Tensor notation
The vorticity equation can be expressed in tensor notation using Einstein's summation convention and the LeviCivita symbol e_{ijk}:
In specific sciences
Atmospheric sciences
In the atmospheric sciences, the vorticity equation can be stated in terms of the absolute vorticity of air with respect to an inertial frame, or of the vorticity with respect to the rotation of the Earth. The absolute version is
Here, η is the polar (z) component of the vorticity, ρ is the atmospheric density, u, v, and w are the components of wind velocity, and ∇_{h} is the 2dimensional (i.e. horizontalcomponentonly) del.
References
 Burr, K. P. "Marine Hydrodynamics, Lecture 9" (PDF). MIT Lectures.
 Manna, Utpal; Sritharan, S. S. (2007). "Lyapunov Functionals and Local Dissipativity for the Vorticity Equation in L^{p} and Besov spaces". Differential and Integral Equations. 20 (5): 581–598.
 Barbu, V.; Sritharan, S. S. (2000). "MAccretive Quantization of the Vorticity Equation" (PDF). In Balakrishnan, A. V. (ed.). SemiGroups of Operators: Theory and Applications. Boston: Birkhauser. pp. 296–303.
 Krigel, A. M. (1983). "Vortex evolution". Geophysical & Astrophysical Fluid Dynamics. 24: 213–223.