Effects of high-frequency and balanced motions on Lagrangian pair dispersion at the ocean surface
Michael Maalouly, Apolline Dekens, Guillaume Lapeyre, Aur\'elien Luigi Serge Ponte, Stefano Berti

TL;DR
This study examines how high-frequency internal gravity waves and balanced motions influence surface particle dispersion in the ocean, revealing that dispersion is mainly governed by nearly-balanced flows at larger scales, with implications for satellite-based measurements.
Contribution
It demonstrates that high-frequency internal gravity waves do not significantly affect relative dispersion, emphasizing the dominant role of nearly-balanced flows at larger scales.
Findings
In winter, dispersion aligns with kinetic energy spectra.
In summer, internal waves dominate small-scale energy.
Satellite measurements may have limitations in estimating dispersion.
Abstract
We investigate the properties of relative dispersion of Lagrangian particles in a global-ocean simulation resolving both inertia-gravity waves (IGW) and meso and submesoscale (M/SM) turbulence. More specifically, we test if the dispersion laws depend on the shape of the Eulerian kinetic energy spectrum, as predicted from quasi-geostrophic turbulence theory. To this end, we focus on two areas, in the Kuroshio Extension and in the Gulf Stream, for which the relative importance of IGW compared to M/SM vary in summer and winter. In winter, Lagrangian statistical indicators return a picture in overall agreement with the shape of the kinetic energy spectrum. Conversely, in summer, when submesoscales are less energetic and higher-frequency internal waves gain importance, the expected relations between dispersion properties and spectra do not seem to hold. This apparent discrepancy is explained…
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Taxonomy
TopicsOceanographic and Atmospheric Processes · Ocean Waves and Remote Sensing · Marine and coastal ecosystems
