Physics:Enstrophy
In fluid dynamics, the enstrophy [math]\displaystyle{ \mathcal{E} }[/math] 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 [math]\displaystyle{ \Omega \subseteq \R^n }[/math] and a once-weakly differentiable vector field [math]\displaystyle{ u \in H^1(\R^n)^n }[/math] which represents a fluid flow, such as a solution to the Navier-Stokes equations, its enstrophy is given by:[1]
[math]\displaystyle{ \mathcal{E}({\bf u}) := \int_\Omega |\nabla \mathbf{u}|^2 \, dx }[/math]
where [math]\displaystyle{ |\nabla \mathbf{u}|^2 = \sum_{i,j=1}^n \left| \partial_i u^j \right|^2 }[/math]. This quantity is the same as the squared seminorm [math]\displaystyle{ |\mathbf{u}|_{H^1(\Omega)^n}^2 }[/math]of the solution in the Sobolev space [math]\displaystyle{ H^1(\Omega)^n }[/math].
Incompressible flow
In the case that the flow is incompressible, or equivalently that [math]\displaystyle{ \nabla \cdot \mathbf{u} = 0 }[/math], the enstrophy can be described as the integral of the square of the vorticity [math]\displaystyle{ \mathbf{\omega} }[/math]:[2]
- [math]\displaystyle{ \mathcal{E}(\boldsymbol \omega) \equiv \int_\Omega |\boldsymbol \omega|^2 \,dx }[/math]
or, in terms of the flow velocity:
- [math]\displaystyle{ \mathcal{E}(\mathbf{u}) \equiv \int_{S} |\nabla \times \mathbf u|^2 \,dS }[/math]
In the context of the incompressible Navier-Stokes equations, enstrophy appears in the following useful result:[1]
- [math]\displaystyle{ \frac{d}{dt} \left( \frac{1}{2} \int_\Omega |\mathbf{u}|^2 \right) = - \nu \mathcal{E}(\mathbf{u}) }[/math]
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 [math]\displaystyle{ \nu }[/math] times the enstrophy.
See also
References
- ↑ 1.0 1.1 Navier-Stokes equations and turbulence. Ciprian Foiaş. Cambridge: Cambridge University Press. 2001. pp. 28–29. ISBN 0-511-03936-0. OCLC 56416088. https://www.worldcat.org/oclc/56416088.
- ↑ Doering, C. R. and Gibbon, J. D. (1995). Applied Analysis of the Navier-Stokes Equations, p. 11, Cambridge University Press, Cambridge. ISBN:052144568-X.
Further reading
- Arakawa, A.; Lamb, V.R. (January 1981). "A Potential Enstrophy and Energy Conserving Scheme for the Shallow Water Equations". Monthly Weather Review 109 (1): 18-36. doi:10.1175/1520-0493(1981)109<0018:APEAEC>2.0.CO;2. ISSN 1520-0493. https://journals.ametsoc.org/view/journals/mwre/109/1/1520-0493_1981_109_0018_apeaec_2_0_co_2.xml.
- Umurhan, O. M.; Regev, O. (December 2004). "Hydrodynamic stability of rotationally supported flows: Linear and nonlinear 2D shearing box results". Astronomy and Astrophysics 427 (3): 855–872. doi:10.1051/0004-6361:20040573. Bibcode: 2004A&A...427..855U.
- Weiss, John (March 1991). "The dynamics of enstrophy transfer in two-dimensional hydrodynamics". Physica D: Nonlinear Phenomena 48 (2–3): 273–294. doi:10.1016/0167-2789(91)90088-Q. Bibcode: 1991PhyD...48..273W.
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