Impact of Deep Water Formation on Antarctic Circumpolar Transport During Gateway Opening

D. R. Munday*, I. Sauermilch, A. Klocker, J. M. Whittaker

*Corresponding author for this work

Research output: Contribution to journalArticleAcademicpeer-review

Abstract

Ambiguity over the Eocene opening times of the Tasman Gateway and Drake Passage makes it difficult to determine the initiation time of the Antarctic Circumpolar Current. If the Tasman Gateway opened later than Drake Passage, then Australia may have prevented the proto-ACC from forming. Recent modeling results have shown that only a relatively weak circumpolar transport results under Eocene surface forcing. This leads to warm and buoyant coastal water around Antarctica, which may impede the formation of deep waters and convective processes. This suggests that a change in deep water formation might be required to increase the density contrast across the Southern Ocean and increase circumpolar transport. Here we use a simple reduced gravity model with two basins, to represent the Atlantic and the Pacific. This fixes the density difference between surface and deep water and allows us to isolate the impact of deep water formation on circumpolar transport. With no obstacle on the southern boundary the circumpolar current increases its transport from 82.3 to 270.0 Sv with deep water formation. Placing an Antipodean landmass on the southern boundary reduces this transport as the landmass increases in size. However, circumpolar flow north of this landmass remains a possibility even without deep water formation. Weak circumpolar transport continues until the basin is completely blocked by the Antipodes. When the Antipodes is instead allowed to split from the southern boundary, circumpolar transport recovers to its unobstructed value. Flow rapidly switches to south of the Antipodes when the gateway is narrow.

Original languageEnglish
Article numbere2022PA004605
JournalPaleoceanography and Paleoclimatology
Volume39
Issue number5
DOIs
Publication statusPublished - May 2024

Bibliographical note

Publisher Copyright:
© 2024. The Author(s).

Funding

DRM was supported by the Natural Environment Research Council (ORCHESTRA, Grant NE/N018095/1). This work used JASMIN, the UK's collaborative data analysis environment (see , Lawrence et al., 2013). Isabel Sauermilch acknowledges funding through the ERC starting Grant n802835 OceaNice. The initial experiments were conducted when DRM was a PDRA at the University of Oxford, supported by the Natural Environment Research Council. This research was partially supported by the Australian Government through the Australian Research Council's Discovery Projects funding scheme (project DP180102280). The authors thank Matthew Huber and three anonymous reviewers whose comments improved the clarity of the paper and led to an improved discussion.

FundersFunder number
British Antarctic SurveyNE/N018095/1
Natural Environment Research Council (ORCHESTRA)
ERC
Natural Environment Research CouncilDP180102280
Australian Government through the Australian Research Council

    Keywords

    • circumpolar transport
    • deep water formation
    • gateway opening

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