Simulation and Scaling of the Turbulent Vertical Heat Transport and Deep-Cycle Turbulence across the Equatorial Pacific Cold Tongue

Author:

Whitt D. B.12ORCID,Cherian D. A.2,Holmes R. M.3456,Bachman S. D.2,Lien R.-C.7,Large W. G.2,Moum J. N.8

Affiliation:

1. a NASA Ames Research Center, Moffett Field, California

2. b National Center for Atmospheric Research, Boulder, Colorado

3. c School of Geosciences, University of Sydney, Sydney, New South Wales, Australia

4. d Climate Change Research Centre, University of New South Wales, Sydney, New South Wales, Australia

5. e School of Mathematics and Statistics, University of New South Wales, Sydney, New South Wales, Australia

6. f ARC Centre of Excellence for Climate Extremes, University of New South Wales, Sydney, New South Wales, Australia

7. g Applied Physics Laboratory, University of Washington, Seattle, Washington

8. h College of Earth, Ocean, and Atmospheric Sciences, Oregon State University, Corvallis, Oregon

Abstract

Abstract Microstructure observations in the Pacific cold tongue reveal that turbulence often penetrates into the thermocline, producing hundreds of watts per square meter of downward heat transport during nighttime and early morning. However, virtually all observations of this deep-cycle turbulence (DCT) are from 0°, 140°W. Here, a hierarchy of ocean process simulations, including submesoscale-permitting regional models and turbulence-permitting large-eddy simulations (LES) embedded in a regional model, provide insight into mixing and DCT at and beyond 0°, 140°W. A regional hindcast quantifies the spatiotemporal variability of subsurface turbulent heat fluxes throughout the cold tongue from 1999 to 2016. Mean subsurface turbulent fluxes are strongest (∼100 W m−2) within 2° of the equator, slightly (∼10 W m−2) stronger in the northern than Southern Hemisphere throughout the cold tongue, and correlated with surface heat fluxes (r2 = 0.7). The seasonal cycle of the subsurface heat flux, which does not covary with the surface heat flux, ranges from 150 W m−2 near the equator to 30 and 10 W m−2 at 4°N and 4°S, respectively. Aseasonal variability of the subsurface heat flux is logarithmically distributed, covaries spatially with the time-mean flux, and is highlighted in 34-day LES of boreal autumn at 0° and 3°N, 140°W. Intense DCT occurs frequently above the undercurrent at 0° and intermittently at 3°N. Daily mean heat fluxes scale with the bulk vertical shear and the wind stress, which together explain ∼90% of the daily variance across both LES. Observational validation of the scaling at 0°, 140°W is encouraging, but observations beyond 0°, 140°W are needed to facilitate refinement of mixing parameterization in ocean models. Significance Statement This work is a fundamental contribution to a broad community effort to improve global long-range weather and climate forecast models used for seasonal to longer-term prediction. Much of the predictability on seasonal time scales is derived from the slow evolution of the upper eastern equatorial Pacific Ocean as it varies between El Niño and La Niña conditions. This study presents state-of-the-art high-resolution regional numerical simulations of ocean turbulence and mixing in the eastern equatorial Pacific. The results inform future planning for field work as well as future efforts to refine the representation of ocean mixing in global forecast models.

Funder

National Oceanic and Atmospheric Administration

Publisher

American Meteorological Society

Subject

Oceanography

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