Submesoscale eddies (those smaller than 50 km) are ubiquitous throughout the ocean, as revealed by satellite infrared images. Diagnosing their impact on ocean energetics from observations remains a challenge. This study analyzes a turbulent field of submesoscale eddies using airborne observations of surface currents and sea surface temperature, with high spatial resolution, collected during the S-MODE experiment in October 2022. Assuming surface current divergence and temperature are homogeneous down to 30 m depth, we show that more than 80% of the upward vertical heat fluxes, reaching ∼227 W m−2, is explained by the smallest resolved eddies, with a size smaller than 15 km. This result emphasizes the contribution of small-scale eddies, poorly represented in numerical models, to the ocean heat budget and, therefore, to the climate system.
Submesoscale eddy contribution to ocean vertical heat flux diagnosed from airborne observations
Torres, H.S., A. Wineteer, E. Rodriguez, J.M. Klein, A. Thompson, D. Perkovic-Martin, M.J. Molemaker, D.J. Hypolite, J. Callies, and J.T. Farrar (2024), Submesoscale eddy contribution to ocean vertical heat flux diagnosed from airborne observations, Geophys. Res. Lett.(submitted).
Abstract
Disclaimer: This material is being kept online for historical purposes. Though accurate at the time of publication, it is no longer being updated. The page may contain broken links or outdated information, and parts may not function in current web browsers. Visit https://espo.nasa.gov for information about our current projects.