Enstrophy Explained

In fluid dynamics, the enstrophy

l{E}

can be interpreted as another type of potential density; or, more concretely, the quantity directly related to the kinetic energy in the flow model that corresponds to dissipation effects in the fluid. It is particularly useful in the study of turbulent flows, and is often identified in the study of thrusters as well as in combustion theory and meteorology.

Given a domain

\Omega\subseteq\Rn

and a once-weakly differentiable vector field

u\inH1(\Rn)n

which represents a fluid flow, such as a solution to the Navier-Stokes equations, its enstrophy is given by:[1] where

|\nablau|2=

n
\sum
i,j=1

\left|\partialiuj\right|2

. This quantity is the same as the squared seminorm
2
|u|
H1(\Omega)n
of the solution in the Sobolev space

H1(\Omega)n

.

Incompressible flow

In the case that the flow is incompressible, or equivalently that

\nablau=0

, the enstrophy can be described as the integral of the square of the vorticity

\omega

:[2]

l{E}(\boldsymbol\omega)\equiv\int\Omega|\boldsymbol\omega|2dx

or, in terms of the flow velocity:

l{E}(u)\equiv\int\Omega|\nabla x u|2dx

In the context of the incompressible Navier-Stokes equations, enstrophy appears in the following useful result:

d
dt

\left(

1
2

\int\Omega|u|2\right)=-\nul{E}(u)

\nu

times the enstrophy.

See also

Further reading

Notes and References

  1. Book: Navier-Stokes equations and turbulence. 2001. Cambridge University Press. Ciprian Foiaş. 0-511-03936-0. Cambridge. 28–29. 56416088.
  2. Doering, C. R. and Gibbon, J. D. (1995). Applied Analysis of the Navier-Stokes Equations, p. 11, Cambridge University Press, Cambridge. .