Turbulent Mixing Variability in an Energetic Standing Meander of the Southern Ocean

Author:

Cyriac Ajitha12,Phillips Helen E.134,Bindoff Nathaniel L.1325,Polzin Kurt6

Affiliation:

1. a Institute for Marine and Antarctic Studies, University of Tasmania, Hobart, Tasmania, Australia

2. d ARC Centre of Excellence in Climate Extremes, Hobart, Tasmania, Australia

3. b Australian Antarctic Program Partnership, University of Tasmania, Hobart, Tasmania, Australia

4. c Australian Centre for Excellence in Antarctic Science, University of Tasmania, Hobart, Tasmania, Australia

5. e CSIRO Marine and Atmospheric Research, Hobart, Tasmania, Australia

6. f Department of Physical Oceanography, Woods Hole Oceanographic Institution, Woods Hole, Massachusetts

Abstract

Abstract This study presents novel observational estimates of turbulent dissipation and mixing in a standing meander between the Southeast Indian Ridge and the Macquarie Ridge in the Southern Ocean. By applying a finescale parameterization on the temperature, salinity, and velocity profiles collected from Electromagnetic Autonomous Profiling Explorer (EM-APEX) floats in the upper 1600 m, we estimated the intensity and spatial distribution of dissipation rate and diapycnal mixing along the float tracks and investigated the sources. The indirect estimates indicate strong spatial and temporal variability of turbulent mixing varying from O(10−6) to O(10−3) m2 s−1 in the upper 1600 m. Elevated turbulent mixing is mostly associated with the Subantarctic Front (SAF) and mesoscale eddies. In the upper 500 m, enhanced mixing is associated with downward-propagating wind-generated near-inertial waves as well as the interaction between cyclonic eddies and upward-propagating internal waves. In the study region, the local topography does not play a role in turbulent mixing in the upper part of the water column, which has similar values in profiles over rough and smooth topography. However, both remotely generated internal tides and lee waves could contribute to the upward-propagating energy. Our results point strongly to the generation of turbulent mixing through the interaction of internal waves and the intense mesoscale eddy field.

Publisher

American Meteorological Society

Subject

Oceanography

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