EGU21-10003
https://doi.org/10.5194/egusphere-egu21-10003
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Ekman-inertial instability

Nicolas Grisouard and Varvara E Zemskova
Nicolas Grisouard and Varvara E Zemskova
  • University of Toronto, Department of Physics, Toronto, Canada (nicolas.grisouard@utoronto.ca)

We report on an instability arising in sub-surface, laterally sheared geostrophic flows. When the lateral shear of a horizontal flow in geostrophic balance has a sign opposite to the Coriolis parameter and exceeds it in magnitude, embedded perturbations are subjected to inertial instability, albeit modified by viscosity. When the perturbation arises from the surface of the fluid, the initial response is akin to a Stokes problem, with an initial flow aligned with the initial perturbation. The perturbation then grows quasi-inertially, rotation deflecting the velocity vector, which adopts a well-defined angle with the mean flow, and viscous stresses, transferring horizontal momentum downward. The combination of rotational and viscous effects in the dynamics of inertial instability prompts us to call this process “Ekman-inertial instability.” While the perturbation initially grows super-inertially, the growth rate then becomes sub-inertial, eventually tending back to the inertial value. The same process repeats downward as time progresses. Ekman-inertial transport aligns with the asymptotic orientation of the flow and grows exactly inertially with time once the initial disturbance has passed. Because of the strongly super-inertial initial growth rate, this instability might compete favourably against other instabilities arising in ocean fronts.

How to cite: Grisouard, N. and Zemskova, V. E.: Ekman-inertial instability, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-10003, https://doi.org/10.5194/egusphere-egu21-10003, 2021.

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