๐”– Bobbio Scriptorium
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The Ekman spiral

โœ Scribed by T. H. Ellison


Book ID
104571816
Publisher
John Wiley and Sons
Year
1955
Tongue
English
Weight
137 KB
Volume
81
Category
Article
ISSN
0035-9009

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โœฆ Synopsis


Abstract

Previous workers have used an eddy viscosity varying with height linearly or according to a power law, when discussing the variation of the wind between the surface and the height at which it (supposedly) attains the geostrophic value, but they have not used the appropriate boundary conditions to obtain the familiar forms for the velocity profile very near the surface. In conditions of neutral stability this profile is given by
where u~*~ = (ฯ„)^1/2^ and k = 0ยท40. Eq. (1) corresponds to an eddy viscosity, K~M~, given by
If this formula is assumed to hold at all heights, and the geostrophic wind is assumed to be uniform and constant, it can be shown that
where u is the component of the wind in the direction of the surface wind and v that perpendicular to it; the suffix G denotes the geostrophic value and f is the Coriolis parameter.


๐Ÿ“œ SIMILAR VOLUMES


The Ekman Spirals
โœ Th. Hesselberg ๐Ÿ“‚ Article ๐Ÿ“… 1954 ๐Ÿ› Springer ๐ŸŒ English โš– 748 KB
Dune trend and the Ekman Spiral
โœ WARREN, A. ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Nature Publishing Group ๐ŸŒ English โš– 267 KB
Ekman spirals for exponential thermal wi
โœ L. J. Mahrt; W. Schwerdtfeger ๐Ÿ“‚ Article ๐Ÿ“… 1970 ๐Ÿ› Springer ๐ŸŒ English โš– 463 KB

The equations for a family of wind spirals are derived with the assumption that the thermal wind in the friction layer decreases exponentially with increasing height. The results are discussed with reference to the flow in the planetary boundary layer over the Antarctic Plateau.