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 i
A numerical study of the nocturnal atmospheric boundary layer
โ Scribed by Yves Delage
- Publisher
- John Wiley and Sons
- Year
- 1974
- Tongue
- English
- Weight
- 617 KB
- Volume
- 100
- Category
- Article
- ISSN
- 0035-9009
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โฆ Synopsis
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 oneโdimensional numerical model. The model uses a turbulent energy equation for the determination of the eddy exchange coefficients, which also involve the local value of the MoninโObukhov length. The surface temperature is prescribed as a function of time and the geostrophic wind is held constant. Results are presented in nondimensional form and cover a wide range of possible values for the external parameters. After several hours of cooling the inversion layer is found to reach a maximum depth, which depends strongly upon the magnitude of the geostrophic wind and, to a lesser extent, on the cooling rate of the ground surface.
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The structure of nocturnal inversions in the first 300 m of the atmosphere is analyzed using observational data from the Boulder Atmospheric Observatory (BAO) from March through June 1981. The temperature profiles show more than one inversion layer 41% of the time during the observational period. Th
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
## Abstract The dynamics of largeโscale, horizontal roll vortices in the neutral planetary boundary layer are investigated by means of a twoโdimensional numerical model. The rolls are assumed to be twoโdimensional and are calculated explicitly, while smallโscale turbulence is parametrized by a mixi