Abstract:Analyses of hydrographic observation data sets revealed that modified Circumpolar Deep Water (mCDW) tends to flood the western flank (73–78°E, 67–68°S) of the Four Ladies Bank (FLB) in Prydz Bay. In this study, we investigated the mechanism responsible for mCDW upwelling over the FLB based on an eddy‐resolving coupled ocean‐sea ice‐ice shelf model in conjunction with the latest high‐accuracy bathymetry. It was found that zonal step‐like declines in the seabed over the FLB are crucial for the mCDW onshore upwel… Show more
“…Although the Antarctic Slope front (ASF) acts as a strong dynamical barrier to the inflow of CDW across the shelf in East Antarctica (Spence et al, ; Thompson et al, ), intrusions of mCDW have been observed in the sea ice growth season (March–August), entering Prydz Bay over Four Ladies Bank (FLB) and occupying the eastern side of the bay following the cyclonic PBG and are directed toward the eastern flank of the AIS (Herraiz‐Borreguero et al, ; Liu et al, ; Williams et al, ). The interaction of the AIS with mCDW heat transport has been clarified by several studies (Herraiz‐Borreguero et al, , ; Wong et al, ), and the AIS net basal melt rate driven by mCDW inflow was estimated at 1.0 ± 0.4 m/year (Herraiz‐Borreguero et al, ), reducing local shelf water density and suppressing its potential contribution to AABW formation (Williams et al, ).…”
The coastal shelf region of East Antarctica is hypothesized to be shielded from the offshore heat of Circumpolar Deep Water (CDW) due to the dynamic barrier of the Antarctic Slope Front. Yet modified CDW (mCDW) intrudes into the coastal environment in key locations, with impacts on dense shelf water formation and ocean/ice shelf interaction that remain largely unquantified. Using moored measurements and conductivity‐temperature‐depth‐instrumented seal hydrographic data collected in Prydz Bay, East Antarctica, we find buoyancy‐driven upwelling of mCDW into the subsurface (~50 m) layer of the southeastern embayment. Wintertime convection extends as deep as 300 m, entraining heat of the upwelled mCDW to the surface. Accumulated sensible heat supply to the surface through deep convection during June–July reduces the potential sea ice production by 45% in the Davis Polynya, demonstrating that stronger/warmer mCDW intrusions onto the shelf will likely reduce the shelf water density and threaten Antarctic Bottom Water formation.
“…Although the Antarctic Slope front (ASF) acts as a strong dynamical barrier to the inflow of CDW across the shelf in East Antarctica (Spence et al, ; Thompson et al, ), intrusions of mCDW have been observed in the sea ice growth season (March–August), entering Prydz Bay over Four Ladies Bank (FLB) and occupying the eastern side of the bay following the cyclonic PBG and are directed toward the eastern flank of the AIS (Herraiz‐Borreguero et al, ; Liu et al, ; Williams et al, ). The interaction of the AIS with mCDW heat transport has been clarified by several studies (Herraiz‐Borreguero et al, , ; Wong et al, ), and the AIS net basal melt rate driven by mCDW inflow was estimated at 1.0 ± 0.4 m/year (Herraiz‐Borreguero et al, ), reducing local shelf water density and suppressing its potential contribution to AABW formation (Williams et al, ).…”
The coastal shelf region of East Antarctica is hypothesized to be shielded from the offshore heat of Circumpolar Deep Water (CDW) due to the dynamic barrier of the Antarctic Slope Front. Yet modified CDW (mCDW) intrudes into the coastal environment in key locations, with impacts on dense shelf water formation and ocean/ice shelf interaction that remain largely unquantified. Using moored measurements and conductivity‐temperature‐depth‐instrumented seal hydrographic data collected in Prydz Bay, East Antarctica, we find buoyancy‐driven upwelling of mCDW into the subsurface (~50 m) layer of the southeastern embayment. Wintertime convection extends as deep as 300 m, entraining heat of the upwelled mCDW to the surface. Accumulated sensible heat supply to the surface through deep convection during June–July reduces the potential sea ice production by 45% in the Davis Polynya, demonstrating that stronger/warmer mCDW intrusions onto the shelf will likely reduce the shelf water density and threaten Antarctic Bottom Water formation.
“…Thus, it can be assumed that ocean circulation and tides are key drivers for sea ice stability in the Southern Ocean. According to, for example, Tamsitt et al (2017) and Liu et al (2018), upwelling of deeper water masses can be expected along the shelf break. Tides apparently have a great influence on the stability of the sea ice.…”
Sea ice is of substantial importance for the Southern Ocean, as it insulates the relatively warm ocean from the cold atmosphere. Due to mechanical stress induced by wind and ocean currents, sea ice leads occur, which are characterized by open water and thin ice causing an increase of energy and moisture fluxes between ocean and atmosphere. Furthermore, they contribute to the ice production and provide a habitat for animals. Thus, it is important to gain information about the temporal and spatial distribution of leads on a circum‐Antarctic scale. So far, no operational data set exists, which provides such information. We use thermal satellite imagery from the Moderate Resolution Imaging Spectroradiometer to derive the predominant lead patterns for 2003–2018, April–September. This study provides first results for the long‐term average lead frequencies in the Southern Ocean and discusses possible links to ocean currents, tides, and the bathymetry.
“…A narrow Antarctic Coastal Current (ACoC), driven by offshore and easterly winds, flows westwards near to the coast (Smith et al, 1984). Intrusion of Modified Circumpolar Deep Water (MCDW) occurs over Four Ladies Bank and eventually flows into the Prydz Bay Gyre and the AIS cavity (Galton-Fenzi et al, 2012;Liu et al, 2018). This MCDW is an important factor in driving basal melting of the AIS (Herraiz-Borreguero et al, 2015).…”
“…Observations from APRES confirm this and show that a seasonal cycle in basal melting is practically nonexistent at the two sampled sites. However, despite the weak observed melting, observations from moorings, ship, and instrumented seals over many years (Guo et al, 2019;Nunes Vaz & Lennon, 1996;Smith et al, 1984;Williams et al, 2010Williams et al, , 2016Wong et al, 1998) and multiple modeling studies (Galton-Fenzi et al, 2012;Liu et al, 2017Liu et al, , 2018 of the Prydz Bay region have shown that MCDW upwells over the Four Ladies Bank and is present close to the coastline in significant quantity. This MCDW has been shown to (in part) drive melting beneath the AIS (Herraiz-Borreguero et al, 2013;Herraiz-Borreguero et al, 2015) and is known to drive strong melt in other locations around Antarctica (e.g., Walker et al, 2013).…”
Section: Weak Basal Melting Beneath the Sørsdal Ice Shelfmentioning
Basal melting of ice shelves is inherently difficult to quantify through direct observations, yet it is a critical factor controlling Antarctic mass balance and global sea-level rise. While much research attention is paid to larger ice shelves and those experiencing the most rapid change, many smaller, unstudied ice shelves offer valuable insights. Here, we investigate the oceanographic conditions and melting beneath the Sørsdal ice shelf, East Antarctica. We present results from the 2018/2019 Sørsdal deployment of the University of Tasmania's autonomous underwater vehicle nupiri muka. Oceanography adjacent to and beneath the ice shelf front shows a cold and relatively saline environment dominated by Winter Water and Dense Shelf Water, while bathymetry measurements show a deep (∼1,200 m) trough running into the ice shelf cavity. Two multiyear deployments of Autonomous Phase-sensitive Radar Echo Sounders on the surface of the ice shelf show weak melt rates (average of 1.6 and 2.3 m yr −1) with low temporal variability. These observations are supported by numerical ocean model and satellite estimates of melting. We speculate that the presence of a ∼825 m thick (350 m to at least 1,175 m) homogeneous layer of cold, dense water blocks access from warmer waters that intrude into Prydz Bay from offshore, resulting in weak melt rates. However, the newly identified trough means that the ice shelf is vulnerable to any decrease in polynya activity that allows warm water to enter the cavity. This could lead to increased basal melting and mass loss through this sector of Antarctica.
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