Linear stability of an oceanic front at finite Rossby number
Subhajit Kar, Roy Barkan, John R. Taylor

TL;DR
This study investigates how finite Rossby numbers influence the linear stability of oceanic fronts, revealing a transition from baroclinic to inertia-critical layer instabilities and emphasizing the importance of shear production in mixed layer dynamics.
Contribution
It provides a systematic linear stability analysis of oceanic fronts across a range of Rossby numbers, highlighting the changing dominant instability mechanisms.
Findings
At low Rossby numbers, baroclinic instability dominates.
As Rossby number increases, inertia-critical layer instability becomes prevalent.
Shear production becomes significant and should be included in models.
Abstract
Submesoscale currents in the ocean's mixed layer (ML), consisting of fronts, eddies, and filaments, are characterized by order one Rossby (Ro) and Richardson (Ri) numbers. These currents play a crucial role in mediating vertical exchange between the surface and ocean interior and in facilitating cross-scale energy transfers. Despite a growing understanding of their generation mechanisms and energy pathways, two fundamental questions remain unresolved - how does a finite Ro modify the dynamics of ML instabilities, and what mechanisms are responsible for ML frontal arrest when Ro is order one. In this study, we address these questions through a linear stability analysis of a two-dimensional, geostrophically adjusted oceanic front based on the analytical model of Ou(1984), which allows systematic exploration across a range of Ro. In the low Ro, order one Ri regime, the most unstable mode…
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Taxonomy
TopicsMethane Hydrates and Related Phenomena · Geology and Paleoclimatology Research · Geomagnetism and Paleomagnetism Studies
