What is it about?
The Ekman boundary layer (EBL) is a central problem in geophysical fluid dynamics that emerges when the pressure gradient force, the Coriolis force, and the frictional force interact in a flow. The unsteady version of the problem, which occurs when these forces are not in equilibrium, is solvable analytically only for a limited set of forcing variability regimes, and the resulting solutions are intricate and not always easy to interpret. In this paper, large-eddy simulations (LESs) of neutral atmospheric EBLs are conducted under various unsteady forcings to reveal the range of physical characteristics of the flow. Subsequently, it is demonstrated that the dynamics of the unsteady EBL can be reduced to a second-order ordinary differential equation that is very similar to the dynamical equation of a damped oscillator, such as a mass–spring–damper system. The validation of the proposed reduced model is performed by comparing its analytical solutions to LES results, revealing very good agreement. The reduced model can be solved for a wide range of variable forcing conditions, and this feature is exploited in the paper to elucidate the physical origin of the inertia (mass), energy storage (spring), and energy dissipation (damper) attributes of Ekman flows.
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Why is it important?
Unsteadiness resulting from the pressure forcing associated in the atmosphere with mesoscale variability and, in particular, the response of the EBL to different time scales of the unsteady geostrophic forcing have been less studied. Other similar approaches can derive solutions for a limited range of conditions and often result in intricate expressions that can be hard to interpret physically. Here we develop simpler analytical solutions to model the wind velocity variations in a wide range of conditions.
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This page is a summary of: Large-Eddy Simulations and Damped-Oscillator Models of the Unsteady Ekman Boundary Layer, Journal of the Atmospheric Sciences, January 2016, American Meteorological Society,
DOI: 10.1175/jas-d-15-0038.1.
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