convective boundary layers
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MAUSAM ◽  
2021 ◽  
Vol 51 (2) ◽  
pp. 169-176
Author(s):  
SAVITA B. MORWAL

Results of an investigation of the Convective Boundary Layer (CBL) structure over the oceanic region in the vicinity of the equator during the summer monsoon season are presented. The data were obtained from stationary research vessels viz., Shirshov, Okean, Shokalsky and Priboy during the MONSOON-77 Experiment.   Variations in structure between convective boundary layers over the four ships with respect to their position about the equator have been studied. The technique of saturation point, mixing line and conserved variable diagrams has been used to bring out these differences. The CBL structure over the four ships showed that in the vicinity of the equator there are no marked differences. However, the analysis carried out for the period of study revealed that the ships situated south of the equator represented more convective activity, higher moisture content and deep layer clouds as compared to the ships which were located at the equator and north of equator. The two ships, located at the equator, showed approximately similar convective boundary layer structure.


AIP Advances ◽  
2020 ◽  
Vol 10 (10) ◽  
pp. 105306
Author(s):  
Keith G. McNaughton ◽  
Subharthi Chowdhuri

2020 ◽  
Vol 77 (10) ◽  
pp. 3619-3630
Author(s):  
Jeremy A. Gibbs ◽  
Evgeni Fedorovich

AbstractWe extend our previous study, which dealt with structure functions of potential temperature fluctuations, and focus on the characteristics of second-order velocity structure functions and corresponding structure parameters in the atmospheric convective boundary layer. We consider the three previously reported methods to compute the structure parameters of turbulent velocity fields: the direct method, the true spectral method, and the approximate spectral method. The methods are evaluated using high-resolution gridded numerical data from large-eddy simulations of shear-free and shear-driven convective boundary layers. Results indicate that the direct and true spectral methods are more suitable than the approximate spectral method, which overestimates the structure parameters of velocity as a result of assuming the inertial-subrange shape of the velocity spectrum for all turbulence scales. Results also suggest that structure parameters of vertical velocity fluctuations are of limited utility because of violations of local isotropy, especially in shear-free convective boundary layers.


2019 ◽  
Vol 76 (12) ◽  
pp. 3697-3715 ◽  
Author(s):  
Armin Haghshenas ◽  
Juan Pedro Mellado ◽  
Moritz Hartmann

Abstract Two zero-order bulk models (ZOMs) are developed for the velocity, buoyancy, and moisture of a cloud-free barotropic convective boundary layer (CBL) that grows into a linearly stratified atmosphere. The models differ in the entrainment closure assumption: in the first one, termed the “energetics-based model,” the negative and positive areas of the buoyancy flux are assumed to match between the model and the actual CBL; in the second one, termed the “geometric-based model,” the modeled CBL depth is assumed to match different definitions of the actual CBL depth. Parameterizations for these properties derived from direct numerical simulation (DNS) are employed as entrainment closure equations. These parameterizations, and hence the resulting models, are free from the potential singularity at finite wind strength that has been a major limitation in previous bulk models. The proposed ZOMs are verified using the DNS data. Model results show that the CBL depths obtained from the energetics-based model and previous ZOMs correspond to the height that marks the transition from the lower to the upper entrainment-zone sublayer; this reference height is few hundred meters above the height of the minimum buoyancy flux. It is also argued that ZOMs, despite their simplicity compared to higher-order models, can accurately represent CBL bulk properties when the relevant features of the actual entrainment zone are considered in the entrainment closures. The vertical structure of the actual entrainment zone, if required, can be constructed a posteriori using the available relationships between the predicted zero-order CBL depth and various definitions of the actual CBL depth.


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