Three-dimensional turbulence occurs mainly in convective clouds and in the atmospheric boundary layer. Two-dimensional turbulence is a model for the statistical features of large-scale flows in the atmosphere. The differences between two- and three-dimensional turbulence are discussed, with a minimum of mathematics, in terms of elementary vorticity dynamics. The influence of the microstructure on the evolution of the large-scale features of the flow field is explored in some detail. A simple rationale is given for ignoring subgrid scale fluxes in numerical weather prediction. (A)
CITATION STYLE
Tennekes, H. (1978). Turbulent flow in two and three dimensions. Bulletin of the American Meteorological Society, 59(1, Jan.1978), 22–28. https://doi.org/10.1175/1520-0477(1978)059<0022:tfitat>2.0.co;2
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