Effects of Wind and Isopycnal Mixing on Southern Ocean Surface Buoyancy Flux and Antarctic Bottom Water Formation

Abstract In coarse resolution ocean models, eddy diffusive effects are parameterized using an isopycnal mixing coefficient, which controls mixing strength along isopycnals. Recent high‐resolution simulations show that increasing the wind stress over the Southern Ocean leads to increased local isopycnal mixing. In this work, we investigate how wind and isopycnal mixing affect surface temperature and salinity in the Southern Ocean and the buoyancy of waters near Antarctica. Using an idealized Massachusetts Institute of Technology general circulation model basin‐channel model, we vary both Southern Ocean wind stress and the isopycnal mixing coefficient independently. We find that when the wind and isopycnal mixing coefficient are small, a strong halocline in the far south prevents AABW formation. Increasing the wind stress and/or isopycnal mixing brings warmer, saltier water to the surface of the Southern Ocean, where it cools, becomes denser, and forms AABW. Increasing the isopycnal mixing coefficient also increases the latitudinal extent of the source waters for AABW formation.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-04-05
DOI
https://doi.org/10.1029/2024gl112133
Citations
1
Primary Topic
Oceanographic and Atmospheric Processes
Type
article
Field-Weighted Citation Impact
1.79

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article

Effects of Wind and Isopycnal Mixing on Southern Ocean Surface Buoyancy Flux and Antarctic Bottom Water Formation

C Spencer Jones, N. Neumann
1 citations
Geophysical Research Letters
Oceanographic and Atmospheric Processes
1.79
article

Effects of Wind and Isopycnal Mixing on Southern Ocean Surface Buoyancy Flux and Antarctic Bottom Water Formation

C Spencer Jones, N. Neumann
article en
1 citations

Abstract

Abstract In coarse resolution ocean models, eddy diffusive effects are parameterized using an isopycnal mixing coefficient, which controls mixing strength along isopycnals. Recent high‐resolution simulations show that increasing the wind stress over the Southern Ocean leads to increased local isopycnal mixing. In this work, we investigate how wind and isopycnal mixing affect surface temperature and salinity in the Southern Ocean and the buoyancy of waters near Antarctica. Using an idealized Massachusetts Institute of Technology general circulation model basin‐channel model, we vary both Southern Ocean wind stress and the isopycnal mixing coefficient independently. We find that when the wind and isopycnal mixing coefficient are small, a strong halocline in the far south prevents AABW formation. Increasing the wind stress and/or isopycnal mixing brings warmer, saltier water to the surface of the Southern Ocean, where it cools, becomes denser, and forms AABW. Increasing the isopycnal mixing coefficient also increases the latitudinal extent of the source waters for AABW formation.

Geophysical Research LettersVol. 52(7)
Texas A&M University (US)
High Performance Research Computing, Texas A and M University
Openalex Percentile: Top 19%
Oceanographic and Atmospheric Processes
1.79
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