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An Improved Model for the Turbulent PBLSecond order turbulence models of the Mellor and Yamada type have been widely used to simulate the PBL. It is however known that these models have several deficiencies. For example, they all predict a critical Richardson number which is about four times smaller than the Large Eddy Simulation (LES) data, they are unable to match the surface data, and they predict a boundary layer height lower than expected. In the present model, we show that these difficulties are all overcome by a single new physical input: the use of the most complete expression for both the pressure-velocity and the pressure-temperature correlations presently available. Each of the new terms represents a physical process that, was not accounted for by previous models. The new model is presented in three different levels according to Mellor and Yamada's terminology, with new, ready-to-use expressions for the turbulent, moments. We show that the new model reproduces several experimental and LES data better than previous models. As far as the PBL is concerned, we show that the model reproduces both the Kansas data as analyzed by Businger et al. in the context of Monin-Obukhov similarity theory for smaller Richardson numbers, as well as the LES and laboratory data up to Richardson numbers of order unity. We also show that the model yields a higher PBL height than the previous models.
Document ID
20010071588
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Cheng, Y.
(NASA Goddard Inst. for Space Studies New York, NY United States)
Canuto, V. M.
(Columbia Univ. New York, NY United States)
Howard, A. M.
(NASA Goddard Inst. for Space Studies New York, NY United States)
Hansen, James E.
Date Acquired
September 7, 2013
Publication Date
January 24, 2001
Subject Category
Geophysics
Report/Patent Number
GCN-01-13
Report Number: GCN-01-13
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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