Drag and heat transfer relations for the planetary boundary layer

Physics

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Scientific paper

A theory is offered for the drag and heat transfer relations in the statistically steady, horizontally homogeneous, diabatic, barotropic planetary boundary layer. The boundary layer is divided into three regions R 1, R 2, and R 3, in which the heights are of the order of magnitude of z 0, L, and h, respectively, where z 0 is the roughness length for either momentum or temperature, L is the Obukhov length, and h is the height of the planetary boundary layer. A matching procedure is used in the overlap zones of regions R 1 and R 2 and of regions R 2 and R 3, assuming that z 0 ≪ L ≪ h. The analysis yields the three similarity functions A(μ), B(μ), and C(μ) of the stability parameter, μ = ϰ u */ fL, where ϰ is von Kármán's constant, u * is the friction velocity at the ground and f is the Coriolis parameter. The results are in agreement with those previously found by Zilitinkevich (1975) for the unstable case, and differ from his results only by the addition of a universal constant for the stable case. Some recent data from atmospheric measurements lend support to the theory and permit the approximate evaluation of universal constants.

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