Investigating the formation of submesoscale structures along mesoscale fronts and estimating kinematic quantities using Lagrangian drifters

dc.contributor.authorLodise, John
dc.contributor.authorÖzgökmen, Tamay
dc.contributor.authorGonçalves, Rafael C.
dc.contributor.authorIskandarani, Mohamed
dc.contributor.authorLund, Björn
dc.contributor.authorHorstmann, Jochen
dc.contributor.authorPoulain, Pierre-Marie
dc.contributor.authorKlymak, Jody
dc.contributor.authorRyan, Edward H.
dc.contributor.authorGuigand, Cedric
dc.date.accessioned2022-12-02T23:47:31Z
dc.date.available2022-12-02T23:47:31Z
dc.date.copyright2020en_US
dc.date.issued2020
dc.description.abstractMuch of the vertical transport near the surface of the ocean, which plays a critical role in the transport of dissolved nutrients and gases, is thought to be associated with ageostrophic submesoscale phenomena. Vertical velocities are challenging not only to model accurately, but also to measure because of how difficult they are to locate in the surface waters of the ocean. Using unique massive drifter releases during the Lagrangian Submesoscale Experiment (LASER) campaign in the Gulf of Mexico and the Coherent Lagrangian Pathways from the Surface Ocean to the Interior (CALYPSO) experiment in the Mediterranean Sea, we investigate the generation of submesoscale structures along two different mesoscale fronts. We use a novel method to project Lagrangian trajectories to Eulerian velocity fields, in order to calculate horizontal velocity gradients at the surface, which are used as a proxy for vertical transport. The velocity reconstruction uses a squared-exponential covariance function, which characterizes velocity correlations in horizontal space and time, and determines the scales of variation using the data itself. SST and towed CTD measurements support the findings revealed by the drifter data. Due to the production of a submesoscale instability eddy in the Gulf of Mexico, convergence magnitudes of up to ~20 times the planetary vorticity, f , are observed, the value of which is almost 3 times larger than that found in the mesoscale dominated Western Mediterranean Sea.en_US
dc.description.reviewstatusRevieweden_US
dc.description.scholarlevelFacultyen_US
dc.description.sponsorshipThis research has been supported by the Gulf of Mexico Research Initiative (grant no. GR009731) and by The Office of Naval Research grant number N000141812138. Rafael Gonçalves was supported under the auspices of the Cooperative Institute for Marine and Atmospheric Studies (CIMAS), a cooperative institute of the University of Miami and NOAA, cooperative agreement NA10OAR4320143. This work was also supported by NOAA/AOML.en_US
dc.identifier.citationLodise, J., Özgökmen, T., Gonçalves, R. C., Iskandarani, M., Lund, B., Horstmann, J., . . . Guigand, C. (2020). “Investigating the formation of submesoscale structures along mesoscale fronts and estimating kinematic quantities using Lagrangian drifters.” Fluids, 5(3), 159. https://doi.org/10.3390/fluids5030159en_US
dc.identifier.urihttps://doi.org/10.3390/fluids5030159
dc.identifier.urihttp://hdl.handle.net/1828/14540
dc.language.isoenen_US
dc.publisherFluidsen_US
dc.subjectmesoscale/submesoscale interaction
dc.subjectkinematics
dc.subjectLagrangian drifters
dc.subject.departmentSchool of Earth and Ocean Sciences
dc.titleInvestigating the formation of submesoscale structures along mesoscale fronts and estimating kinematic quantities using Lagrangian driftersen_US
dc.typeArticleen_US

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