Impact of Deep Water Formation on Antarctic Circumpolar Transport During
Gateway Opening
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 (ACC). If the Tasman Gateway opened later
than Drake Passage, then Australia may have prevented the proto-ACC from
forming. Recent modelling 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.