An oceanic ultra-violet catastrophe, wave-particle duality and a strongly nonlinear concept for geophysical turbulence

dc.contributor.author Polzin, Kurt L.
dc.contributor.author Lvov, Yuri V.
dc.date.accessioned 2017-08-02T19:00:39Z
dc.date.available 2017-08-02T19:00:39Z
dc.date.issued 2017-06-29
dc.description © The Author(s), 2017. This article is distributed under the terms of the Creative Commons Attribution License. The definitive version was published in Fluids 2 (2017): 36, doi:10.3390/fluids2030036. en_US
dc.description.abstract There is no theoretical underpinning that successfully explains how turbulent mixing is fed by wave breaking associated with nonlinear wave-wave interactions in the background oceanic internal wavefield. We address this conundrum using one-dimensional ray tracing simulations to investigate interactions between high frequency internal waves and inertial oscillations in the extreme scale separated limit known as “Induced Diffusion”. Here, estimates of phase locking are used to define a resonant process (a resonant well) and a non-resonant process that results in stochastic jumps. The small amplitude limit consists of jumps that are small compared to the scale of the resonant well. The ray tracing simulations are used to estimate the first and second moments of a wave packet’s vertical wavenumber as it evolves from an initial condition. These moments are compared with predictions obtained from the diffusive approximation to a self-consistent kinetic equation derived in the ‘Direct Interaction Approximation’. Results indicate that the first and second moments of the two systems evolve in a nearly identical manner when the inertial field has amplitudes an order of magnitude smaller than oceanic values. At realistic (oceanic) amplitudes, though, the second moment estimated from the ray tracing simulations is inhibited. The transition is explained by the stochastic jumps obtaining the characteristic size of the resonant well. We interpret this transition as an adiabatic ‘saturation’ process which changes the nominal background wavefield from supporting no mixing to the point where that background wavefield defines the normalization for oceanic mixing models. en_US
dc.description.sponsorship Kurt L. Polzin gratefully acknowledges support from Woods Hole Oceanographic Institution’s Investment in Science Program (WHOI’s ISP) program. The authors gratefully acknowledge support from a collaborative National Science Foundation grant, award Nos. 1634644 (KP) and 1635866 (YVL). en_US
dc.identifier.citation Fluids 2 (2017): 36 en_US
dc.identifier.doi 10.3390/fluids2030036
dc.identifier.uri https://hdl.handle.net/1912/9147
dc.language.iso en_US en_US
dc.publisher MDPI AG en_US
dc.relation.uri https://doi.org/10.3390/fluids2030036
dc.rights Attribution 4.0 International *
dc.rights.uri http://creativecommons.org/licenses/by/4.0/ *
dc.subject Wave-wave interactions en_US
dc.subject Internal waves en_US
dc.subject Mixing en_US
dc.subject Anderson localization en_US
dc.title An oceanic ultra-violet catastrophe, wave-particle duality and a strongly nonlinear concept for geophysical turbulence en_US
dc.type Article en_US
dspace.entity.type Publication
relation.isAuthorOfPublication f8ec2386-fa4b-4626-9285-6ced466be58f
relation.isAuthorOfPublication a9a5fe65-fb66-4f6c-b675-aa0c2f1b10ed
relation.isAuthorOfPublication.latestForDiscovery f8ec2386-fa4b-4626-9285-6ced466be58f
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