Turbulent flow in two and three dimensions.

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Abstract

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)

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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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