The theoretical distribution of wind in the planetary boundary layer with circular isobars

Details The theoretical distribution of wind in the planetary boundary layer with circular isobars The theoretical distribution of wind in the planetary boundary layer with circular isobars

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983bolme..26..209m&link_type=abstract

Boundary-Layer Meteorology, Volume 26, Issue 3, pp.209-226

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3

Scientific paper

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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