NASA NTRS · 20000093326
New Third-Order Moments for the PBL
Abstract
Turbulent convection is inherently non-local and a primary condition for a successful treatment of the PBL is a reliable model of non-locality. In the dynamic equations governing the convective flux, turbulent kinetic energy, etc, non-locality enters through the third-order moments, TOMs. Since the simplest form, the so-called down gradient approximation (DGA , severely underestimates the TOMs (by up to an order of magnitude), a more physical model is needed. In 1994, an analytical model was presented which was derived directly from the dynamical equations for the TOMs. It considerably improved the DGA but was a bit cumbersome to use. Here, we present a new analytic expression for the TOMs which is considerably simpler than the 1994 expression and which at the same time yields a much better fit to the LES data.
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Canuto, V. M., Cheng, Y., Howard, A., Hansen, James E.. 2000-01-01. New Third-Order Moments for the PBL. https://ntrs.nasa.gov/citations/20000093326
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