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Published July 2018 | Published
Journal Article Open

Partitioning of Kinetic Energy in the Arctic Ocean's Beaufort Gyre

Abstract

Kinetic energy (KE) in the Arctic Ocean's Beaufort Gyre is dominated by the mesoscale eddy field that plays a central role in the transport of freshwater, heat, and biogeochemical tracers. Understanding Beaufort Gyre KE variability sheds light on how this freshwater reservoir responds to wind forcing and sea ice and ocean changes. The evolution and fate of mesoscale eddies relate to energy pathways in the ocean (e.g., the exchange of energy between barotropic and baroclinic modes). Mooring measurements of horizontal velocities in the Beaufort Gyre are analyzed to partition KE into barotropic and baroclinic modes and explore their evolution. We find that a significant fraction of water column KE is in the barotropic and the first two baroclinic modes. We explain this energy partitioning by quantifying the energy transfer coefficients between the vertical modes using the quasi‐geostrophic potential vorticity conservation equations with a specific background stratification observed in the Beaufort Gyre. We find that the quasi‐geostrophic vertical mode interactions uphold the persistence of KE in the first two baroclinic modes, consistent with observations. Our results explain the specific role of halocline structure on KE evolution in the gyre and suggest depressed transfer to the barotropic mode. This limits the capacity for frictional dissipation at the sea floor and suggests that energy dissipation via sea ice‐ocean drag may be prominent.

Additional Information

© 2018 American Geophysical Union. Received 2 APR 2018; Accepted 31 MAY 2018; Accepted article online 20 JUN 2018; Published online 10 JUL 2018. This article also appears in: Forum for Arctic Modeling and Observational Synthesis (FAMOS) 2: Beaufort Gyre phenomenon. Mooring data were collected and made available by the Beaufort Gyre Exploration Program based at the Woods Hole Oceanographic Institution (http://www.whoi.edu/beaufortgyre) in collaboration with researchers from Fisheries and Oceans Canada at the Institute of Ocean Sciences. Funding was provided by the National Science Foundation Division of Polar Programs under award 1107623. We appreciate the support and helpful scientific discussions associated with the Forum for Arctic Modeling and Observational Synthesis (FAMOS) and the FAMOS School for Young Arctic Scientists. We thank Andrey Proshutinsky and John Marshall for helpful comments.

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Published - Zhao_et_al-2018-Journal_of_Geophysical_Research_3A_Oceans.pdf

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Additional details

Created:
August 21, 2023
Modified:
October 18, 2023