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Log-Normal Turbulence Dissipation in Global Ocean Models

Brodie Pearson and Baylor Fox-Kemper
Phys. Rev. Lett. 120, 094501 – Published 26 February 2018
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Abstract

Data from turbulent numerical simulations of the global ocean demonstrate that the dissipation of kinetic energy obeys a nearly log-normal distribution even at large horizontal scales O(10km). As the horizontal scales of resolved turbulence are larger than the ocean is deep, the Kolmogorov-Yaglom theory for intermittency in 3D homogeneous, isotropic turbulence cannot apply; instead, the down-scale potential enstrophy cascade of quasigeostrophic turbulence should. Yet, energy dissipation obeys approximate log-normality—robustly across depths, seasons, regions, and subgrid schemes. The distribution parameters, skewness and kurtosis, show small systematic departures from log-normality with depth and subgrid friction schemes. Log-normality suggests that a few high-dissipation locations dominate the integrated energy and enstrophy budgets, which should be taken into account when making inferences from simplified models and inferring global energy budgets from sparse observations.

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  • Received 25 October 2017

DOI:https://doi.org/10.1103/PhysRevLett.120.094501

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Fluid Dynamics

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Intermittent Turbulence in a Global Ocean Model

Published 26 February 2018

A large-scale model of ocean dynamics finds intermittent behavior that may have implications for how the ocean’s energy budget is assessed.

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Authors & Affiliations

Brodie Pearson and Baylor Fox-Kemper

  • Department of Earth, Environmental and Planetary Sciences, Brown University, Providence, Rhode Island 02906, USA

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Issue

Vol. 120, Iss. 9 — 2 March 2018

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