This is a Preprint and has not been peer reviewed. This is version 1 of this Preprint.
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Abstract
In the ocean, submesoscale flows tend to undergo several hydrodynamic instabilities. In particular, Inertial Instability (InI) and Ekman-Inertial Instability (EII) are known to develop in geostrophically balanced barotropic flows whose lateral shear is larger in magnitude and opposite in sign to the Coriolis parameter. Although these instabilities share some elements, their dynamical nature can lead to fundamental differences. However, the current analytical description of EII is one-dimensional, which makes it difficult to compare against InI in a more realistic scenario. To overcome this limitation, we conduct two-dimensional numerical simulations of both InI and EII in a submesoscale jet and explore the induced vertical flow, the growth rate, and the energetics of each instability. Furthermore, we investigate the sensitivity of our results to variations in the minimum Rossby number of the jet. We find that EII grows faster than InI and induces stronger vertical flow, especially near the surface. Both instabilities radiate inertial waves away from the current, and these waves predominantly propagate across the anticyclonic side of the jet. Finally, when the instabilities weaken, the fluid reaches a stable state that is remarkably similar in both cases. This study highlights the similarities and differences between InI and EII and provides further insight into the mechanism behind EII that makes it capable of outcompeting other submesoscale instabilities.
DOI
https://doi.org/10.31223/X56X3Q
Subjects
Oceanography, Oceanography and Atmospheric Sciences and Meteorology, Physical Sciences and Mathematics
Keywords
Flow instability, Submesoscale, Rotating flows, Shear flows
Dates
Published: 2024-08-29 03:39
Last Updated: 2024-08-29 10:39
License
CC BY Attribution 4.0 International
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Conflict of interest statement:
None
Data Availability (Reason not available):
The data that support the findings of this article will be publicly available in the coming weeks.
There are no comments or no comments have been made public for this article.