Balance in non-hydrostatic rotating shallow-water flows

Unsteady nonlinear shallow-water flows typically emit inertia-gravity waves through a process called spontaneous adjustment-emission. This process has been studied extensively within the rotating shallow-water model, the simplest geophysical model having the required capability. Here, we consider what happens when the hydrostatic assumption underpinning the shallow-water model is dropped. This assumption is in fact not necessary for the derivation of a two-dimensional or single-layer flow model. All one needs is that the horizontal flow field be independent of height in the fluid layer. Then, vertical averaging yields a single-layer flow model with the full range of expected conservation laws, similar to the shallow-water model yet allowing for non-hydrostatic effects. These effects become important for horizontal scales comparable to or less than the depth of the fluid layer. In a rotating flow, such scales may be activated if the Rossby deformation length (the ratio of the characteristic gravity-wave speed to the Coriolis frequency) is comparable to the depth of the fluid layer. Then, the range of frequencies supporting inertia-gravity waves is compressed, and the group velocity of these waves is reduced. We find that this change in wave properties has the effect of strongly suppressing spontaneous adjustment-emission and trapping inertia-gravity waves near regions of relatively strong circulation.

Automated summary

The article discusses obtaining a single-layer flow model with non-hydrostatic effects when the hydrostatic assumption of the shallow-water model is dropped. In rotating flows, non-hydrostatic effects become important when the Rossby deformation length is comparable to the depth of the fluid layer, leading to compression of inertia-gravity waves and reduction in group velocity.