Enstrophy

In fluid dynamics, the enstrophy \mathcal{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 \R^n and a once-weakly differentiable vector field u \in H^1(\R^n)^n which represents a fluid flow, such as a solution to the Navier-Stokes equations, its enstrophy is given by:{{Cite book|url=https://www.worldcat.org/oclc/56416088|title=Navier-Stokes equations and turbulence|date=2001|publisher=Cambridge University Press|others=Ciprian Foiaş|isbn=0-511-03936-0|location=Cambridge|pages=28–29|oclc=56416088}}{{Equation box 1|cellpadding|border|indent=:|equation= \mathcal{E}({\bf u}) := \int_\Omega |\nabla \mathbf{u}|^2 \, d \mathbf x |border colour=#0073CF|background colour=#F5FFFA}}where |\nabla \mathbf{u}|^2 = \sum_{i,j=1}^n \left| \partial_i u^j \right|^2 . This quantity is the same as the squared seminorm |\mathbf{u}|_{H^1(\Omega)^n}^2of the solution in the Sobolev space H^1(\Omega)^n.

Incompressible flow

In the case that the flow is incompressible, or equivalently that \nabla \cdot \mathbf{u} = 0 , the enstrophy can be described as the integral of the square of the vorticity \mathbf{\omega} :Doering, C. R. and Gibbon, J. D. (1995). Applied Analysis of the Navier-Stokes Equations, p. 11, Cambridge University Press, Cambridge. {{ISBN|052144568-X}}.

: \mathcal{E}(\boldsymbol \omega) \equiv \int_\Omega |\boldsymbol \omega|^2 \,d \mathbf x

or, in terms of the flow velocity:

: \mathcal{E}(\mathbf{u}) \equiv \int_\Omega |\nabla \times \mathbf u|^2 \,d \mathbf x

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

: \frac{d}{dt} \left( \frac{1}{2} \int_\Omega |\mathbf{u}|^2 \right) = - \nu \mathcal{E}(\mathbf{u})

The quantity in parentheses on the left is the kinetic energy in the flow, so the result says that energy declines proportional to the kinematic viscosity \nu times the enstrophy.

See also

References

{{Reflist}}

Further reading

  • {{cite journal |last1=Arakawa |first1=A. |last2=Lamb |first2=V.R. |title=A Potential Enstrophy and Energy Conserving Scheme for the Shallow Water Equations |journal=Monthly Weather Review |date=January 1981 |volume=109 |issue=1 |pages=18–36 |doi=10.1175/1520-0493(1981)109<0018:APEAEC>2.0.CO;2 |issn=1520-0493 |arxiv= |bibcode= 1981MWRv..109...18A|s2cid=|doi-access=free }}
  • {{cite journal |last1=Umurhan |first1=O. M. |last2=Regev |first2=O. |title=Hydrodynamic stability of rotationally supported flows: Linear and nonlinear 2D shearing box results |journal=Astronomy and Astrophysics |date=December 2004 |volume=427 |issue=3 |pages=855–872 |doi=10.1051/0004-6361:20040573 |arxiv=astro-ph/0404020 |bibcode=2004A&A...427..855U |s2cid=15418079}}
  • {{cite journal|last1=Weiss|first1=John|title=The dynamics of enstrophy transfer in two-dimensional hydrodynamics|journal=Physica D: Nonlinear Phenomena|date=March 1991|volume=48|issue=2–3|pages=273–294|doi=10.1016/0167-2789(91)90088-Q|bibcode = 1991PhyD...48..273W }}

Category:Continuum mechanics

Category:Fluid dynamics

Category:Turbulence