scholarly journals Early westward flow across the Tasman Gateway

2015 ◽  
Vol 11 (5) ◽  
pp. 5021-5048
Author(s):  
W. P. Sijp ◽  
A. S. von der Heydt ◽  
P. K. Bijl
Keyword(s):  
Southern Ocean ◽  
Ocean Circulation ◽  
Surface Waters ◽  
Middle Eocene ◽  
Drake Passage ◽  
Easterly Wind ◽  
Wind Pattern ◽  
Sw Pacific ◽  
Field Evidence ◽  
Set Up

Abstract. The timing and role in ocean circulation and climate of the opening of Southern Ocean gateways is as yet elusive. Recent micropaleontological studies suggest the onset of throughflow of surface waters from the SW Pacific into the Australo-Antarctic Gulf through a southern shallow opening of the Tasman Gateway from 49–50 Ma onwards. Here, we present the first model results specific to the early-to-middle Eocene where, in agreement with the field evidence, southerly shallow opening of the Tasman Gateway indeed causes a westward flow across the Tasman Gateway. As a result, modelled estimates of dinoflagellate biogeography are in agreement with the recent findings. Crucially, in this situation where Australia is still situated far south and almost attached to Antarctica, the Drake Passage must be sufficiently restricted to allow the prevailing easterly wind pattern to set up this southerly restricted westward flow. In contrast, an open Drake Passage, to 517 m depth, leads to an eastward flow, even when the Tasman Gateway and the Australo-Antarctic gulf are entirely contained within the latitudes of easterly wind.

scholarly journals Model simulations of early westward flow across the Tasman Gateway during the early Eocene

2016 ◽  
Vol 12 (4) ◽  
pp. 807-817 ◽  
Author(s):  
Willem P. Sijp ◽  
Anna S. von der Heydt ◽  
Peter K. Bijl
Keyword(s):  
Ocean Circulation ◽  
Surface Waters ◽  
Middle Eocene ◽  
Drake Passage ◽  
Easterly Wind ◽  
Wind Pattern ◽  
Sw Pacific ◽  
Field Evidence ◽  
Circumpolar Current ◽  
Set Up

Abstract. The timing and role in ocean circulation and climate of the opening of Southern Ocean gateways is as yet elusive. Recent micropalaeontological studies suggest the onset of westward throughflow of surface waters from the SW Pacific into the Australo-Antarctic Gulf through a southern shallow opening of the Tasman Gateway from 49–50 Ma onwards, a direction that is counter to the present-day eastward-flowing Antarctic Circumpolar Current. Here, we present the first model results specific to the early-to-middle Eocene where, in agreement with the field evidence, southerly shallow opening of the Tasman Gateway indeed causes a westward flow across the Tasman Gateway. As a result, modelled estimates of dinoflagellate biogeography are in agreement with the recent findings. Crucially, in this situation where Australia is still situated far south and almost attached to Antarctica, the Drake Passage must be sufficiently restricted to allow the prevailing easterly wind pattern to set up this southerly restricted westward flow. In contrast, an open Drake Passage, up to 517 m deep, leads to an eastward flow, even when the Tasman Gateway and the Australo-Antarctic gulf are entirely contained within the latitudes of easterly wind.

scholarly journals Surface-circulation change in the Southern Ocean across the Middle Eocene Climatic Optimum: inferences from dinoflagellate cysts and biomarker paleothermometry

2019 ◽  
Author(s):  
Margot J. Cramwinckel ◽  
Lineke Woelders ◽  
Emiel P. Huurdeman ◽  
Francien Peterse ◽  
Stephen J. Gallagher ◽  
...  
Keyword(s):  
Climate Change ◽  
Southern Ocean ◽  
Ocean Circulation ◽  
Middle Eocene ◽  
Chemical Properties ◽  
Spatiotemporal Distribution ◽  
Surface Currents ◽  
Dinoflagellate Cysts ◽  
Physico Chemical ◽  
Climatic Optimum

Abstract. Global climate cooled from the early Eocene hothouse (~ 52–50 Ma) to the latest Eocene (~ 34 Ma). At the same time, the tectonic evolution of the Southern Ocean was characterized by the opening and deepening of circum-Antarctic gateways, which affected both surface- and deep-ocean circulation. The Tasman Gateway played a key role in regulating ocean throughflow between Australia and Antarctica. Southern Ocean surface currents through and around the Tasman Gateway have left recognizable tracers in the spatiotemporal distribution of plankton fossils, including organic-walled dinoflagellate cysts. This spatiotemporal distribution depends on physico-chemical properties of the water masses in which these organisms thrived. The degree to which the geographic path of surface currents (primarily controlled by tectonism) or their physico-chemical properties (significantly impacted by climate) have controlled the composition of the fossil assemblages has, however, remained unclear. In fact, it is yet poorly understood to what extent oceanographic response as a whole was dictated by climate change, independent of tectonics-induced oceanographic changes that operate on longer time scales. To disentangle the effects of tectonism and climate in the southwest Pacific Ocean, we target a climatic deviation from the long-term Eocene cooling trend, a 500 thousand year long global warming phase termed the Middle Eocene Climatic Optimum (MECO; ~ 40 Ma). The MECO warming is unrelated to regional tectonism, and thus provides a test case to investigate the oceans physiochemical response to climate change only. We reconstruct changes in surface-water circulation and temperature in and around the Tasman Gateway during the MECO through new palynological and organic geochemical records from the central Tasman Gateway (Ocean Drilling Program Site 1170), the Otway Basin (southeastern Australia) and the Hampden Section (New Zealand). Our results confirm that dinocyst communities track tectonically driven circulation patterns, yet the variability within these communities can be driven by superimposed temperature change. Together with published results from the east of the Tasman Gateway, our results suggest that as surface-ocean temperatures rose, the East Australian Current extended further southward during the peak of MECO warmth. Simultaneous with high sea-surface temperatures in the Tasman Gateway area, pollen assemblages indicate warm temperate rainforests with paratropical elements along the southeastern margin of Australia. Finally, based on new age constraints we suggest that a regional southeast Australian transgression might have been caused by sea-level rise during MECO.

An Austral radiolarian biozonation for the Paleogene

Stratigraphy ◽  
2020 ◽  
pp. 213-278
Author(s):  
Christopher J. Hollis ◽  
Kristina M. Pascher ◽  
Annika Sanfilippo ◽  
Akiko Nishimura ◽  
Shin-ichi Kamikuri ◽  
...  
Keyword(s):  
Indian Ocean ◽  
Southern Ocean ◽  
High Latitude ◽  
Middle Eocene ◽  
Primary Study ◽  
Low Latitude ◽  
Sw Pacific ◽  
Index Species ◽  
Study Sites ◽  
Radiolarian Assemblages

ABSTRACT: We have integrated southern mid- and high-latitude (Austral) radiolarian biozonations with the well-established low-latitude (Tropical) biozonation using new biostratigraphic and magnetostratigraphic constraints on radiolarian bioevents in the Southwest (SW) Pacific, Southeast (SE) Indian and Northwest (NW) Atlantic Oceans. Our primary study sites include Mead Stream, New Zealand, and DSDP Sites 277 and 207 (SW Pacific; 45-54 degrees South at 50 Ma), ODP Site 752 and IODP Site U1514 (SE Indian; 50 degrees South at 50 Ma), and IODP Site U1403 (NW Atlantic; 30 degrees North at 50 Ma). The Austral and Tropical zonal schemes have been calibrated to GPTS2020. We introduce new zonal codes to rectify current confusion surrounding use of "RP" zones. Austral zones are codified as "RPA" zones and Tropical zones are codified as "RPT". Our study finds that radiolarian datums are generally isochronous within the mid-latitude SW Pacific and SE Indian Oceans from Paleocene to middle Eocene and are also isochronous in the high-latitude Southern Ocean (>60 degrees South paleolatitude) over the late middle Eocene to Oligocene interval of overlap. Older radiolarian assemblages are not known from the Southern Ocean. Early to middle Paleocene radiolarian assemblages in the SE Indian Ocean (zones RPA2-RPA5) differ from coeval SW Pacific assemblages by lacking significant numbers of Cretaceous survivors. The reasons for this difference are uncertain. Although the late Paleocene to Eocene radiolarian assemblages in the SW Pacific and SE Indian Ocean lack many low-latitude index species, the timing of Indian Ocean bioevents agrees better with low-latitude biozonations than the SW Pacific, suggesting a stronger connection with low-latitude watermasses. Assemblages from NW Atlantic IODP Site U1403 include numerous low-latitude index species and can be correlated with zones RPT6-RPT13. Many of the species transitions in biostratigraphically important Eocene lineages, however, occur later than in lower latitudes.

scholarly journals Surface sediment characteristics related to provenance and ocean circulation in the Drake Passage sector of the Southern Ocean

2019 ◽  
Vol 154 ◽  
pp. 103135 ◽  
Author(s):  
Shuzhuang Wu ◽  
Gerhard Kuhn ◽  
Bernhard Diekmann ◽  
Lester Lembke-Jene ◽  
Ralf Tiedemann ◽  
...  
Keyword(s):  
Southern Ocean ◽  
Ocean Circulation ◽  
Surface Sediment ◽  
Drake Passage ◽  
Sediment Characteristics

scholarly journals Surface-circulation change in the southwest Pacific Ocean across the Middle Eocene Climatic Optimum: inferences from dinoflagellate cysts and biomarker paleothermometry

2020 ◽  
Vol 16 (5) ◽  
pp. 1667-1689
Author(s):  
Margot J. Cramwinckel ◽  
Lineke Woelders ◽  
Emiel P. Huurdeman ◽  
Francien Peterse ◽  
Stephen J. Gallagher ◽  
...  
Keyword(s):  
Climate Change ◽  
Pacific Ocean ◽  
Southern Ocean ◽  
Ocean Circulation ◽  
Middle Eocene ◽  
Spatiotemporal Distribution ◽  
Ocean Currents ◽  
Surface Currents ◽  
Surface Ocean

Abstract. Global climate cooled from the early Eocene hothouse (∼52–50 Ma) to the latest Eocene (∼34 Ma). At the same time, the tectonic evolution of the Southern Ocean was characterized by the opening and deepening of circum-Antarctic gateways, which affected both surface- and deep-ocean circulation. The Tasmanian Gateway played a key role in regulating ocean throughflow between Australia and Antarctica. Southern Ocean surface currents through and around the Tasmanian Gateway have left recognizable tracers in the spatiotemporal distribution of plankton fossils, including organic-walled dinoflagellate cysts. This spatiotemporal distribution depends on both the physicochemical properties of the water masses and the path of surface-ocean currents. The extent to which climate and tectonics have influenced the distribution and composition of surface currents and thus fossil assemblages has, however, remained unclear. In particular, the contribution of climate change to oceanographic changes, superimposed on long-term and gradual changes induced by tectonics, is still poorly understood. To disentangle the effects of tectonism and climate in the southwest Pacific Ocean, we target a climatic deviation from the long-term Eocene cooling trend: the Middle Eocene Climatic Optimum (MECO; ∼40 Ma). This 500 kyr phase of global warming was unrelated to regional tectonism, and thus provides a test case to investigate the ocean's physicochemical response to climate change alone. We reconstruct changes in surface-water circulation and temperature in and around the Tasmanian Gateway during the MECO through new palynological and organic geochemical records from the central Tasmanian Gateway (Ocean Drilling Program Site 1170), the Otway Basin (southeastern Australia), and the Hampden Beach section (New Zealand). Our results confirm that dinocyst communities track specific surface-ocean currents, yet the variability within the communities can be driven by superimposed temperature change. Together with published results from the east of the Tasmanian Gateway, our new results suggest a shift in surface-ocean circulation during the peak of MECO warmth. Simultaneous with high sea-surface temperatures in the Tasmanian Gateway area, pollen assemblages indicate warm temperate rainforests with paratropical elements along the southeastern margin of Australia. Finally, based on new age constraints, we suggest that a regional southeast Australian transgression might have been coincident with the MECO.

scholarly journals Campbell Plateau: A major control on the SW Pacific sector of the Southern Ocean circulation

2017 ◽  
Author(s):  
Aitana Forcén-Vázquez ◽  
Michael J. M. Williams ◽  
Melissa Bowen ◽  
Lionel Carter ◽  
Helen Bostock
Keyword(s):  
Southern Ocean ◽  
Ocean Circulation ◽  
Intermediate Water ◽  
The South ◽  
Mode Water ◽  
The North ◽  
Sw Pacific ◽  
Consistent Picture ◽  
Southward Extension ◽  
Subantarctic Region

Abstract. New Zealand’s subantarctic region is a dynamic oceanographic zone with the Subtropical Front (STF) to the north and the Subantarctic Front (SAF) to the south. Both the fronts and their associated currents are strongly influenced by topography: the South Island of New Zealand and the Chatham Rise for the STF, and Macquarie Ridge and Campbell Plateau for the SAF. Here for the first time we present a consistent picture across the subantarctic region of the relationships between front positions, bathymetry and water mass structure using eight high resolution oceanographic sections that span the region. Our results show that the northwest side of Campbell Plateau is comparatively warm due to a southward extension of the STF over the plateau. The SAF is steered south and east by Macquarie Ridge and Campbell Plateau, with waters originating in the SAF also found north of the plateau in the Bounty Trough. Subantarctic Mode Water (SAMW) formation is confirmed to exist south of the plateau on the northern side of the SAF in winter, while on Campbell Plateau a deep reservoir persists into the following autumn. Antarctic Intermediate Water (AAIW) is observed in the deeper regions around the edges of the plateau, but not on the plateau, confirming that the waters on the plateau are effectively isolated from AAIW and deeper water masses that typify the open Southern Ocean waters.

scholarly journals Eddy-Induced Modulation of Turbulent Dissipation over Rough Topography in the Southern Ocean

2013 ◽  
Vol 43 (11) ◽  
pp. 2288-2308 ◽  
Author(s):  
J. Alexander Brearley ◽  
Katy L. Sheen ◽  
Alberto C. Naveira Garabato ◽  
David A. Smeed ◽  
Stephanie Waterman
Keyword(s):  
Southern Ocean ◽  
Internal Wave ◽  
Ocean Circulation ◽  
Wave Energy ◽  
Bottom Topography ◽  
Temporal Correlation ◽  
Drake Passage ◽  
Wave Radiation ◽  
Bottom Current ◽  
Turbulent Dissipation

Abstract Mesoscale eddies are universal features of the ocean circulation, yet the processes by which their energy is dissipated remain poorly understood. One hypothesis argues that the interaction of strong geostrophic flows with rough bottom topography effects an energy transfer between eddies and internal waves, with the breaking of these waves causing locally elevated dissipation focused near the sea floor. This study uses hydrographic and velocity data from a 1-yr mooring cluster deployment in the Southern Ocean to test this hypothesis. The moorings were located over a small (~10 km) topographic obstacle to the east of Drake Passage in a region of high eddy kinetic energy, and one was equipped with an ADCP at 2800-m depth from which internal wave shear variance and dissipation rates were calculated. Examination of the ADCP time series revealed a predominance of upward-propagating internal wave energy and a significant correlation (r = 0.45) between shear variance levels and subinertial near-bottom current speeds. Periods of strong near-bottom flow coincided with increased convergence of eddy-induced interfacial form stress in the bottom 1500 m. Predictions of internal wave energy radiation were made from theory using measured near-bottom current speeds, and the mean value of wave radiation (5.3 mW m−2) was sufficient to support the dissipated power calculated from the ADCP. A significant temporal correlation was also observed between radiated and dissipated power. Given the ubiquity of strong eddy flows and rough topography in the Southern Ocean, the transfer from eddy to internal wave energy is likely to be an important term in closing the ocean energy budget.

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