A Numerical Study of Second-Order Turbulent Moments in the Stably Stratified Nocturnal Boundary Layer

Zhu Ping; Xu Xiaojin; Li Xingsheng

doi:10.1007/BF02657510

Impact Factor: 5.8

Volume 9 Issue 2

Mar. 1992

Article Contents

Article > ADVANCES IN ATMOSPHERIC SCIENCES > 1992 > 9(2): 201-212

A Numerical Study of Second-Order Turbulent Moments in the Stably Stratified Nocturnal Boundary Layer

1.
Beijing Institute of Meteorology,Beijing Institute of Meteorology,Academy of Meteorological Science, SMA

doi: 10.1007/BF02657510

Abstract
References
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Abstract:
The structures and the vertical profiles of turbulent variance and covariance of the stably stratified boundary layer (SBL) are simulated with a second-order closure turbulence model. The results confirm that the vertical profiles of the dimensionless turbulence variance and covariance can be well represented by the form F = A(1 - Z / h)x. Here h is the height of SBL. and both exponent a and coefficient A are the functions of terrain, baroclinicity, radiation cooling and the state of temporal development of SBL. Comparing with Minnesota and Cabauw experiment data, we have analysed the value of a and expounded the main reasons that great difference in a exists among different literatures.
References

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Manuscript History

Manuscript received: 10 March 1992

Manuscript revised: 10 March 1992

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

A Numerical Study of Second-Order Turbulent Moments in the Stably Stratified Nocturnal Boundary Layer

1. Beijing Institute of Meteorology,Beijing Institute of Meteorology,Academy of Meteorological Science, SMA

Manuscript received: 1992-03-10
Manuscript revised: 1992-03-10

Abstract: The structures and the vertical profiles of turbulent variance and covariance of the stably stratified boundary layer (SBL) are simulated with a second-order closure turbulence model. The results confirm that the vertical profiles of the dimensionless turbulence variance and covariance can be well represented by the form F = A(1 - Z / h)x. Here h is the height of SBL. and both exponent a and coefficient A are the functions of terrain, baroclinicity, radiation cooling and the state of temporal development of SBL. Comparing with Minnesota and Cabauw experiment data, we have analysed the value of a and expounded the main reasons that great difference in a exists among different literatures.