This afternoon all of the models that we have heard fall in the same
class; namely, local closures. First-order local closure (K-theory or
eddy diffusivity) models the momentum fluxes as down-gradient of
the mean momentum. The second-order local closure models the
third moments as down-gradient of the local second moments, or
local mean variables.
There is another completely different class of modeling or class of
closure, and that is non-local turbulence closure. I mentioned
before about the transilient matrix that describes the mixing
between different points separated a finite distance in space. One
can parameterize this matrix in terms of mean flow state or mean
flow instability. When you do that, you can then make forecasts of
the mean field in a turbulent flow that takes into account this nonlocal
mixing.
That has been done. For the ocean, we found results as good as
third-order local closure. For the atmosphere, results were as good
as second-order local closure. We've used it in three-dimensional
weather forecast models covering the whole United States. This is a
new concept of non-local closure, which is different from all the
other local closures.
When would you want to consider using a non-local kind of closure?
Well, if any of you are dealing with turbulent flow that has a
spectrum of eddy sizes where your greatest energy is in the largest
wavelengths, or if you are dealing with turbulent flow that has large
structures in it that are causing non-local mixing, then you might
want to consider a non-local turbulence closure