Submesoscale turbulence in the upper ocean

dc.contributor.author Callies, Joern
dc.date.accessioned 2015-10-20T17:41:58Z
dc.date.available 2015-10-20T17:41:58Z
dc.date.issued 2016-02
dc.description Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution en_US
dc.description.abstract Submesoscale flows, current systems 1–100 km in horizontal extent, are increasingly coming into focus as an important component of upper-ocean dynamics. A range of processes have been proposed to energize submesoscale flows, but which process dominates in reality must be determined observationally. We diagnose from observed flow statistics that in the thermocline the dynamics in the submesoscale range transition from geostrophic turbulence at large scales to inertia–gravity waves at small scales, with the transition scale depending dramatically on geographic location. A similar transition is shown to occur in the atmosphere, suggesting intriguing similarities between atmospheric and oceanic dynamics.We furthermore diagnose from upper-ocean observations a seasonal cycle in submesoscale turbulence: fronts and currents are more energetic in the deep wintertime mixed layer than in the summertime seasonal thermocline. This seasonal cycle hints at the importance of baroclinic mixed layer instabilities in energizing submesoscale turbulence in winter. To better understand this energization, three aspects of the dynamics of baroclinic mixed layer instabilities are investigated. First, we formulate a quasigeostrophic model that describes the linear and nonlinear evolution of these instabilities. The simple model reproduces the observed wintertime distribution of energy across scales and depth, suggesting it captures the essence of how the submesoscale range is energized in winter. Second, we investigate how baroclinic instabilities are affected by convection, which is generated by atmospheric forcing and dominates the mixed layer dynamics at small scales. It is found that baroclinic instabilities are remarkably resilient to the presence of convection and develop even when rapid overturns keep the mixed layer unstratified. Third, we discuss the restratification induced by baroclinic mixed layer instabilities. We show that the rate of restratification depends on characteristics of the baroclinic eddies themselves, a dependence not captured by a previously proposed parameterization. These insights sharpen our understanding of submesoscale dynamics and can help focus future inquiry into whether and how submesoscale flows influence the ocean’s role in climate. en_US
dc.description.sponsorship National Science Foundation through OCE-0825376, OCE-0849233, OCE-1024198, OCE-1233832, and OCE-0961713 as well as by the Office of Naval Research through N00014-09-1-0458. en_US
dc.format.mimetype application/pdf
dc.identifier.citation Callies, J. (2016). Submesoscale turbulence in the upper ocean [Doctoral thesis, Massachusetts Institute of Technology and Woods Hole Oceanographic Institution]. Woods Hole Open Access Server. https://doi.org/10.1575/1912/7570
dc.identifier.doi 10.1575/1912/7570
dc.identifier.uri https://hdl.handle.net/1912/7570
dc.language.iso en_US en_US
dc.publisher Massachusetts Institute of Technology and Woods Hole Oceanographic Institution en_US
dc.relation.ispartofseries WHOI Theses en_US
dc.title Submesoscale turbulence in the upper ocean en_US
dc.type Thesis en_US
dspace.entity.type Publication
relation.isAuthorOfPublication dd8f545e-14f6-46ba-99dd-5d277446a319
relation.isAuthorOfPublication.latestForDiscovery dd8f545e-14f6-46ba-99dd-5d277446a319
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