Deep Convection as the Key to the Transition From Eocene to Modern Antarctic Circumpolar Current

被引:2
作者
Xing, Qianjiang [1 ]
Klocker, Andreas [2 ]
Munday, David [3 ]
Whittaker, Joanne [1 ]
机构
[1] Univ Tasmania, Inst Marine & Antarct Studies, Hobart, Australia
[2] NORCE Norwegian Res Ctr, Bjerknes Ctr Climate Res, Bergen, Norway
[3] British Antarctic Survey, Cambridge, England
基金
澳大利亚研究理事会;
关键词
surface buoyancy forcing; deep convection; Eocene; ACC; SOUTHERN-OCEAN; DRAKE PASSAGE; CIRCULATION; TRANSPORT; SENSITIVITY; GLACIATION; CLIMATE; EDDIES; ONSET;
D O I
10.1029/2023GL104847
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
From the Eocene (similar to 50 million years ago) to today, Southern Ocean circulation has evolved from the existence of two ocean gyres to the dominance of the Antarctic Circumpolar Current (ACC). It has generally been thought that the opening of Southern Ocean gateways in the late Eocene, in addition to the alignment of westerly winds with these gateways or the presence of the Antarctic ice sheet, was a sufficient requirement for the transition to an ACC of similar strength to its modern equivalent. Nevertheless, models representing these changes produce a much weaker ACC. Here we show, using an eddying ocean model, that the missing ingredient in the transition to a modern ACC is deep convection around the Antarctic continent. This deep convection is caused by cold temperatures and high salinities due to sea-ice production around the Antarctic continent, leading to both the formation of Antarctic Bottom Water and a modern-strength ACC. The evolution of ocean circulation from the early Southern Ocean around 50 million years ago to today has seen much debate over the past decades. The main characteristic of the modern Southern Ocean is the prevalence of the Antarctic Circumpolar Current (ACC), the world's strongest current. In the past it has been thought that the deepening of ocean gateways, and changes in the strength and location of winds, led to an ACC of similar strength to its modern equivalent. Nevertheless, ocean models simulating these changes typically reproduce an ACC with less than a third of the modern ACC's strength. Here we show that the missing ingredient in the transition to a modern ACC is deep convection around the Antarctic continent. Deep convection is due to a combination of cooling and increase in salinity by sea ice formation which allows for water at the ocean surface to become denser than the water below, leading to the mixing of the water column to great depths. This deep convection allows for the ocean to be energized, leading to a modern-strength Antarctic Circumpolar Current. A cool climate around the Antarctic continent is therefore crucial for the development of a modern-strength Antarctic Circumpolar Current. Deep convection is able to drive a strong Antarctic Circumpolar Current (ACC)Surface cooling and sea ice formation are crucial drivers of this deep convectionACC similar to a rim current around convective sites, energizing ocean circulation
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页数:11
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