## Abstract The evolution of the structure of the atmospheric boundary layer during the cooling phase of the diurnal cycle is studied with the help of a oneβdimensional numerical model. The model uses a turbulent energy equation for the determination of the eddy exchange coefficients, which also in
A numerical model study of the structure and similarity scaling of the nocturnal boundary layer (NBL)
β Scribed by A. Lacser; S. P. S. Arya
- Publisher
- Springer
- Year
- 1986
- Tongue
- English
- Weight
- 814 KB
- Volume
- 35
- Category
- Article
- ISSN
- 0006-8314
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β¦ Synopsis
A one-dimensional numerical model based on the equations of mean motion and turbulent kinetic energy (TKE), with Delage's (1974) mixing-length parameterization has been used to simulate the mean and turbulent structure ofthe evolving stably stratified nocturnal boundary layer (NBL). The model also includes a predictive equation for the surface temperature and longwave radiational cooling effects.
In the absence of advective and gravity wave effects, it is found that the model-simulated structure, after a few hours of evolution, could be ordered fairly well by a similarity scaling (u *0, 0*0, L,, and h) based on surface fluxes and the NBL height. Simple expressions are suggested to describe the normalized profiles of momentum and heat fluxes, TKE, eddy-viscosity and energy dissipation. A good ordering of the same variables is also achieved by a local scaling (U * , 0*, and L) based on the height-dependent local fluxes. The normalized TKE, eddy viscosity and energy dissipation are unique functions of z/L and approach constant values as z/L + co, where L is the local Monin-Obukhov length. These constants are close to the values predicted for the surface layer as z/L + co, thus suggesting that the Monin-Obukhov similarity theory can be extended to the whole NBL, by using the local (height-dependent) scales in place of surface-layer scales. The observed NBL structure has been shown to follow local similarity (Nieuwstadt, 1984).
π SIMILAR VOLUMES
A one-dimensional model based on the equations of mean motion and turbulent kinetic energy (TKE) with a mixing-length closure scheme has been developed to simulate the turbulence structure of the evolving stably stratified nocturnal boundary layer (NBL). The model also includes a predictive equation
In an effort to describe the basic vertical structure of the nocturnal boundary layer, observations from four experiments are analyzed. During the night, the depth of significant cooling appears to increase with time while the depth of the turbulence and height of the low level wind maximum tend to
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