Planetary boundary layer (PBL) flows are known to exhibit fundamental differences depending on the relative combination of wind shear and buoyancy forces. Four large-eddy simulations (LESs) spanning the shear and buoyancy flow regimes were generated; two correspond to the extreme cases of shear and buoyancy-driven PBLs, while the other two represent intermediate PBLs where both forces are important. The extreme cases are used to highlight and quantify the basic differences between shear and convective PBLs in: 1) flow structures, 2) overall statistics, and 3) turbulent kinetic energy (TKE) budget distributions. Results from the two intermediate LES cases are used to develop and verify a velocity scaling and a TKE budget model, which are proposed for the intermediate PBL. -from Authors
CITATION STYLE
Chin-Hoh Moeng, & Sullivan, P. P. (1994). A comparison of shear- and buoyancy-driven planetary boundary layer flows. Journal of the Atmospheric Sciences, 51(7), 999–1022. https://doi.org/10.1175/1520-0469(1994)051<0999:acosab>2.0.co;2
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