Abstract
The equations of motions are solved for concentric circular flow in the planetary boundary layer (PBL) under the assumption of K = l 2|∂v/∂z| and gradient wind independent of radius r. The theoretical distribution of wind is obtained for r ≥ 300 km. Other parameters of the PBL are also calculated. Finally, equilibrium of the forces in the PBL is analyzed.
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Ming, Z. The theoretical distribution of wind in the planetary boundary layer with circular isobars. Boundary-Layer Meteorol 26, 209–226 (1983). https://doi.org/10.1007/BF00121399
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DOI: https://doi.org/10.1007/BF00121399