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New Third-Order Moments for the PBLTurbulent 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.
Document ID
20000093326
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Canuto, V. M.
(NASA Goddard Inst. for Space Studies New York, NY United States)
Cheng, Y.
(NASA Goddard Inst. for Space Studies New York, NY United States)
Howard, A.
(NASA Goddard Inst. for Space Studies New York, NY United States)
Hansen, James E.
Date Acquired
September 7, 2013
Publication Date
January 1, 2000
Subject Category
Geophysics
Report/Patent Number
GCN-00-17
Report Number: GCN-00-17
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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