Origin, Signature and Palaeoclimatic Influence of the Antarctic Circumpolar Current
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Variability in the Location. of the Antarctic Polar Front (90 °
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 102, NO. C13, PAGES 27,825-27,833, DECEMBER 15, !997 Variability in the location.of the Antarctic Polar Front (90ø- 20øW) from satellite sea surface temperature data J. Keith Moore, Mark R. Abbott, and James G. Richman Collegeof Oceanicand AtmosphericSciences, Oregon State University, Corvallis Abstract. The path of the AntarcticPolar Front (PF) is mappedusing satellite sea surfacetemperature data from the NOAA/NASA Pathfinderprogram. The mean path and variabilityof the PF are stronglyinfluenced by bathymetry.Meandering intensity is weaker where the bathymetryis steeplysloped and increasesin areaswhere the bottom is relativelyflat. There is an inverserelationship between meandering intensity and both the width of the front and the changein temperatureacross it. There is a persistent,large separationbetween the surfaceand subsurfaceexpressions of the PF at Ewing Bank on the Falkland Plateau. 1. Introduction of meanderingjets and fronts hasbeen done previouslyfor the PF [Legeckis,1977] and other strongfrontal systems[Hansen TheAntarctic Polar Front (PF) is a strongjet within t•e and Maul, 1970; Olsonet al., 1983; Cornilion, 1986]. Antarctic CircumpolarCurrent (ACG), which flowseastward Satellite altimeter data has shown that there is little zonal continuouslyaround Antarctica [Nowlin and Klinck, 1986].The coherencein the variabilityof the ACC [Fu and Chelton,1984; PF, also known as the Antarctic Convergence,is the location Sandwelland Zhang, 1989; Chelton et al., 1990; Gille, 1994; where Antarctic surfacewaters movingto the north sink rap- Gille and Kelly,1996]. These studies emphasize the importance idly belowSubantarctic waters [Deacon, 1933, 1937].Thus the of local and regionalinstabilities [Chelton et al., 1990;Gille and PF is a regionof elevatedcurrent speeds and stronghorizontal Kelly,1996]. -
The Undiscovered Oil and Gas of Antarctica
DEPARTMENT OF THE INTERIOR U.S. Geological Survey The Undiscovered Oil and Gas of Antarctica by John Kingston^ OPEN-FILE REPORT 91-597 This report is preliminary and has not been reviewed for conformity with U.S. Geological Survey editorial standards or with the North American Stratigraphic Code. Any use of trade, product, or firm names is for descriptive purposes only and does not imply endorsement by the U.S. Government. ^Santa Barbara, California CONTENTS Page Abstract ....................................................... 1 Introduction ................................................... 2 Size of area .............................................. 2 Premise and problems of petroleum recoverability .......... 2 Previous investigations and petroleum assessments ......... 2 Methods of assessment ..................................... 4 Regional geology and petroleum occurrence ...................... 6 Assessment by play analysis .................................... 13 Rifted continental margin provinces ....................... 13 General; the south Australia rifted margin analog .... 13 Antarctica-Australia rift province ................... 17 Antarctica-India rift province ....................... 20 Antarctica-Africa rift province ...................... 24 Antarctica-Falkland rift province .................... 24 Interior rift provinces ................................... 30 General .............................................. 30 Ross sea interior rift province ...................... 30 Weddell sea interior rift province .................. -
Modification and Pathways of Southern Ocean Deep Waters in the Scotia
Deep-Sea Research I 49 (2002) 681–705 Modification and pathways of Southern Ocean Deep Waters in the Scotia Sea Alberto C. Naveira Garabatoa,*, Karen J. Heywooda, David P. Stevensb a School of Environmental Sciences, University of East Anglia, Norwich NR4 7TJ, UK b School of Mathematics, University of East Anglia, Norwich NR4 7TJ, UK Received 11 September 2000; received in revised form 11 June 2001; accepted 23 October 2001 Abstract An unprecedented high-quality, quasi-synoptic hydrographic data set collected during the ALBATROSS cruise along the rim of the Scotia Sea is examined to describe the pathways of the deep water masses flowing through the region, and to quantify changes in their properties as they cross the sea. Owing to sparse sampling of the northern and southern boundaries of the basin, the modification and pathways of deep water masses in the Scotia Sea had remained poorly documented despite their global significance. Weddell Sea Deep Water (WSDW) of two distinct types is observed spilling over the South Scotia Ridge to the west and east of the western edge of the Orkney Passage. The colder and fresher type in the west, recently ventilated in the northern Antarctic Peninsula, flows westward to Drake Passage along the southern margin of the Scotia Sea while mixing intensely with eastward-flowing Circumpolar Deep Water (CDW) of the antarctic circumpolar current (ACC). Although a small fraction of the other WSDW type also spreads westward to Drake Passage, the greater part escapes the Scotia Sea eastward through the Georgia Passage and flows into the Malvinas Chasm via a deep gap northeast of South Georgia. -
Chapter 4 Tectonic Reconstructions of the Southernmost Andes and the Scotia Sea During the Opening of the Drake Passage
123 Chapter 4 Tectonic reconstructions of the Southernmost Andes and the Scotia Sea during the opening of the Drake Passage Graeme Eagles Alfred Wegener Institute, Helmholtz Centre for Marine and Polar Research, Bre- merhaven, Germany e-mail: [email protected] Abstract Study of the tectonic development of the Scotia Sea region started with basic lithological and structural studies of outcrop geology in Tierra del Fuego and the Antarctic Peninsula. To 19th and early 20th cen- tury geologists, the results of these studies suggested the presence of a submerged orocline running around the margins of the Scotia Sea. Subse- quent increases in detailed knowledge about the fragmentary outcrop ge- ology from islands distributed around the margins of the Scotia Sea, and later their interpretation in light of the plate tectonic paradigm, led to large modifications in the hypothesis such that by the present day the concept of oroclinal bending in the region persists only in vestigial form. Of the early comparative lithostratigraphic work in the region, only the likenesses be- tween Jurassic—Cretaceous basin floor and fill sequences in South Geor- gia and Tierra del Fuego are regarded as strong enough to be useful in plate kinematic reconstruction by permitting the interpretation of those re- gions’ contiguity in mid-Mesozoic times. Marine and satellite geophysical data sets reveal features of the remaining, submerged, 98% of the Scotia 124 Sea region between the outcrops. These data enable a more detailed and quantitative approach to the region’s plate kinematics. In contrast to long- used interpretations of the outcrop geology, these data do not prescribe the proximity of South Georgia to Tierra del Fuego in any past period. -
Diffuse Spectral Reflectance-Derived Pliocene and Pleistocene Periodicity from Weddell Sea, Antarctica Sediment Cores
Wesleyan University The Honors College Diffuse Spectral Reflectance-derived Pliocene and Pleistocene Periodicity from Weddell Sea, Antarctica Sediment Cores by Tavo Tomás True-Alcalá Class of 2015 A thesis submitted to the faculty of Wesleyan University in partial fulfillment of the requirements for the Degree of Bachelor of Arts with Departmental Honors in Earth and Environmental Sciences Middletown, Connecticut April, 2015 Table of Contents List of Figures------------------------------------------------------------------------------IV Abstract----------------------------------------------------------------------------------------V Acknowledgements-----------------------------------------------------------------------VI 1. Introduction------------------------------------------------------------------------------1 1.1. Project Context-------------------------------------------------------------------------1 1.2. Antarctic Glacial History-------------------------------------------------------------5 1.3. Pliocene--------------------------------------------------------------------------------11 1.4. Pleistocene-----------------------------------------------------------------------------13 1.5. Weddell Sea---------------------------------------------------------------------------14 1.6. Site & Cores---------------------------------------------------------------------------19 1.7. Project Goals-------------------------------------------------------------------------22 2. Methodology----------------------------------------------------------------------------23 -
Article Size, 12 Nm Pore Size; YMC Collision Energy 15, 22.5, and 30; Isolation Window 1.0 M/Z)
Biogeosciences, 18, 3485–3504, 2021 https://doi.org/10.5194/bg-18-3485-2021 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Archaeal intact polar lipids in polar waters: a comparison between the Amundsen and Scotia seas Charlotte L. Spencer-Jones1, Erin L. McClymont1, Nicole J. Bale2, Ellen C. Hopmans2, Stefan Schouten2,3, Juliane Müller4, E. Povl Abrahamsen5, Claire Allen5, Torsten Bickert6, Claus-Dieter Hillenbrand5, Elaine Mawbey5, Victoria Peck5, Aleksandra Svalova7, and James A. Smith5 1Department of Geography, Durham University, Lower Mountjoy, South Road, Durham, DH1 3LE, UK 2NIOZ Royal Netherlands Institute for Sea Research, Department of Marine Microbiology and Biogeochemistry, P.O. Box 59, 1790 AB Den Burg, Texel, the Netherlands 3Department of Earth Sciences, Utrecht University, Utrecht, the Netherlands 4Alfred Wegener Institute, Helmholtz Centre for Polar and Marine Research, 27568 Bremerhaven, Germany 5British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 0ET, UK 6MARUM – Center for Marine Environmental Sciences, University of Bremen, Leobener Str. 8, 28359, Bremen, Germany 7School of Natural and Environmental Sciences, Newcastle University, Newcastle-upon-Tyne, NE1 7RU, UK Correspondence: Charlotte L. Spencer-Jones ([email protected]) Received: 7 September 2020 – Discussion started: 5 November 2020 Revised: 3 March 2021 – Accepted: 23 March 2021 – Published: 11 June 2021 Abstract. The West Antarctic Ice Sheet (WAIS) is one of compassing the sub-Antarctic front through to the southern the largest potential sources of future sea-level rise, with boundary of the Antarctic Circumpolar Current. IPL-GDGTs glaciers draining the WAIS thinning at an accelerating rate with low cyclic diversity were detected throughout the water over the past 40 years. -
In Shackleton's Footsteps
In Shackleton’s Footsteps 20 March – 06 April 2019 | Polar Pioneer About Us Aurora Expeditions embodies the spirit of adventure, travelling to some of the most wild and adventure and discovery. Our highly experienced expedition team of naturalists, historians and remote places on our planet. With over 27 years’ experience, our small group voyages allow for destination specialists are passionate and knowledgeable – they are the secret to a fulfilling a truly intimate experience with nature. and successful voyage. Our expeditions push the boundaries with flexible and innovative itineraries, exciting wildlife Whilst we are dedicated to providing a ‘trip of a lifetime’, we are also deeply committed to experiences and fascinating lectures. You’ll share your adventure with a group of like-minded education and preservation of the environment. Our aim is to travel respectfully, creating souls in a relaxed, casual atmosphere while making the most of every opportunity for lifelong ambassadors for the protection of our destinations. DAY 1 | Wednesday 20 March 2019 Ushuaia, Beagle Channel Position: 21:50 hours Course: 84° Wind Speed: 5 knots Barometer: 1007.9 hPa & falling Latitude: 54°55’ S Speed: 9.4 knots Wind Direction: E Air Temp: 11°C Longitude: 67°26’ W Sea Temp: 9°C Finally, we were here, in Ushuaia aboard a sturdy ice-strengthened vessel. At the wharf Gary Our Argentinian pilot climbed aboard and at 1900 we cast off lines and eased away from the and Robyn ticked off names, nabbed our passports and sent us off to Kathrine and Scott for a wharf. What a feeling! The thriving city of Ushuaia receded as we motored eastward down the quick photo before boarding Polar Pioneer. -
Protection for the Weddell Sea Effort Would Continue Momentum, Safeguard Vital Southern Ocean Waters
A map from Oct 2017 Protection for the Weddell Sea Effort would continue momentum, safeguard vital Southern Ocean waters 48.4 48.6 48.2 Maud Rise Astrid Ridge 48.5 Weddell Sea Marine Protected Area Proposal:a General Protection Zone Fisheries Research Zone Special Protection Zone Weddell Sea CCAMLR management area 48.1 CCAMLR subareas Important Bird Areasb Antarctic Seamountsc Peninsula Sponge distributiond Ice shelf Conservation value of area:e <20% 20-40% 40-60% 60-80% 80-100% Sources: aAlfred Wegener Institute, “Weddell Sea: 8 Reasons for a Marine Protected Area” (2016), https://www.awi.de/fileadmin/user_upload/AWI/Ueber_uns/ Service/Presse/2016/4_Quartal/KM_Weddellmeer_MPA/WEB_UK_Factsheet_Weddellmeer.pdf; bC.M. Harris et al., “Important Bird Areas in Antarctica: 2014 Summary,” BirdLife International and Environmental Research & Assessment Ltd.; cChris Yesson et al., “Knolls and Seamounts in the World Ocean: Links to Shape, KML, and Data Files,” PANGAEA (2011), https://doi.org/10.1594/PANGAEA.757563; dUnpublished sponge distribution in Weddell Sea MPA planning area provided by the Alfred Wegener Institute; eK. Teschke et al., “Scientific Background Document in Support of the Development of a CCAMLR MPA in the Weddell Sea (Antarctica)—Part C: Data Analysis and MPA Scenario Development” (2016), http://epic.awi.de/41178; Marxan “summed solution” represents the percentage of times an area was selected for protection Overview The Commission for the Conservation of Antarctic Marine Living Resources (CCAMLR) is considering a proposal that would create a marine reserve in the Weddell Sea covering 700,000 square miles (1.8 million square kilometers). The Weddell Sea is a remote, ice-covered embayment east of the Antarctic Peninsula, and one of the most pristine marine ecosystems in the world. -
Physical Drivers of Phytoplankton Bloom Initiation in the Southern Ocean's Scotia Sea
UC San Diego UC San Diego Previously Published Works Title Physical Drivers of Phytoplankton Bloom Initiation in the Southern Ocean's Scotia Sea Permalink https://escholarship.org/uc/item/9tz4q3pc Journal JOURNAL OF GEOPHYSICAL RESEARCH-OCEANS, 124(8) ISSN 2169-9275 Authors Prend, Channing J Gille, Sarah T Talley, Lynne D et al. Publication Date 2019-08-01 DOI 10.1029/2019JC015162 Peer reviewed eScholarship.org Powered by the California Digital Library University of California RESEARCH ARTICLE Physical Drivers of Phytoplankton Bloom Initiation 10.1029/2019JC015162 in the Southern Ocean's Scotia Sea Key Points: Channing J. Prend1 , Sarah T. Gille1 , Lynne D. Talley1 , B. Greg Mitchell1 , • Shallow mixed layers in the Scotia 1 1 Sea support the earliest and largest Isabella Rosso , and Matthew R. Mazloff offshore spring phytoplankton 1 bloom in the Southern Ocean Scripps Institution of Oceanography, La Jolla, CA, USA • About 10% of the water in the bloom region is advected from the Weddell Sea, which helps set the unique Abstract The Scotia Sea is the site of one of the largest spring phytoplankton blooms in the Southern fi strati cation Ocean. Past studies suggest that shelf‐iron inputs are responsible for the high productivity in this region, • Vertical transport associated with a stratified Taylor column may but the physical mechanisms that initiate and sustain the bloom are not well understood. Analysis of enhance productivity by supplying profiling float data from 2002 to 2017 shows that the Scotia Sea has an unusually shallow mixed‐layer depth subsurface iron to the euphotic zone during the transition from winter to spring, allowing the region to support a bloom earlier in the season than elsewhere in the Antarctic Circumpolar Current. -
Evaluation of Sea-Ice Thickness from Four Reanalyses in the Antarctic Weddell
https://doi.org/10.5194/tc-2020-71 Preprint. Discussion started: 6 April 2020 c Author(s) 2020. CC BY 4.0 License. Evaluation of Sea-Ice Thickness from four reanalyses in the Antarctic Weddell Sea Qian Shi1,2, Qinghua Yang1,2, Longjiang Mu3,2, Jinfei Wang1,2, François Massonnet4, Matthew Mazloff5 1School of Atmospheric Sciences and Guangdong Province Key Laboratory for Climate Change and Natural Disaster Studies, 5 Sun Yat-sen University, Zhuhai 519082, China 2Southern Marine Science and Engineering Guangdong Laboratory (Zhuhai), Zhuhai 519082, China 3Alfred Wegener Institute Helmholtz Centre for Polar and Marine Research, Bremerhaven 27570, Germany 4Georges Lemaître Centre for Earth and Climate Research, Earth and Life Institute, Université catholique de Louvain, Louvain‐ la‐Neuve, Belgium 10 5Scripps Institution of Oceanography, University of California, San Diego, CA, USA Correspondence to: [email protected] and [email protected] Abstract. Ocean-sea ice coupled models constrained by varied observations provide different ice thickness estimates in the Antarctic. We evaluate contemporary monthly ice thickness from four reanalyses in the Weddell Sea, the German contribution of the Estimating the Circulation and Climate of the Ocean project, Version 2 (GECCO2), the Southern Ocean State Estimate 15 (SOSE), the Nucleus for European Modelling of the Ocean (NEMO) based ocean-ice model (called NEMO-EnKF), and the Global Ice-Ocean Modeling and Assimilation System (GIOMAS), and with reference observations from ICESat-1, Envisat, upward looking sonars and visual ship-based sea-ice observations. Compared with ICESat-1 altimetry and in situ observations, all reanalyses underestimate ice thickness near the coast of the western Weddell Sea, even though ICESat-1 and visual observations may be biased low. -
Chapter 6 Antarctic Oceanography the Region of the World Ocean Bordering on Antarctica Is Unique in Many Respects. First of All
Chapter 6 Antarctic oceanography The region of the world ocean bordering on Antarctica is unique in many respects. First of all, it is the only region where the flow of water can continue all around the globe nearly unhindered and the circulation therefore comes closest to the situation in the atmosphere. Secondly, the permanent thermocline (the interface z = H(x,y) of Figure 3.1) reaches the surface in the Subtropical Convergence (Figure 5.5) and does not extend into the polar regions; temperature differences between the sea surface and the ocean floor close to the continent are below 1°C and generally do not exceed 5°C, i.e. 20% of the difference found in 1 the tropics (Figure 6.1). What this means is that our 1 /2 layer ocean model cannot be applied to the seas around Antarctica. Fig. 6.1. Temperature profiles for different climatic regions near 150°W (Pacific Ocean). (a) tropical (5°S), (b) subtropical (35°S), (c) subpolar (50°S), (d) polar (55°S). The temperature scale is correct for the polar profile; other profiles are shifted successively by 1°C. Note the shallowness of the warm surface layer and the absence of the permanent thermocline in the polar region. Data from Osborne et al. (1991). It may seem strange that having spent five chapters on a discussion of temperate and tropical ocean dynamics, we now begin our regional discussion with a region that does not fit the earlier picture. However, our earlier discussion is not entirely irrelevant; it taught us how to get an idea of a region's dynamics by identifying the important forces and looking at their balance. -
The Age and Origin of the Central Scotia Sea
Geophysical Journal International Geophys. J. Int. (2010) 183, 587–600 doi: 10.1111/j.1365-246X.2010.04781.x The age and origin of the central Scotia Sea Graeme Eagles Department of Earth Sciences, Royal Holloway University of London, Egham, Surrey TW20 0EX, UK. E-mail: [email protected] Accepted 2010 August 18. Received 2010 July 6; in original form 2010 May 7 SUMMARY Opening of the Drake Passage gateway between the Pacific and Atlantic oceans has been linked in various ways to Cenozoic climate changes. From the oceanic floor of Drake Passage, the largest of the remaining uncertainties in understanding this opening is in the timing and process of the opening of the central Scotia Sea. All but one of the available constraints on the age of the central Scotia Sea is diagnostic of, or consistent with, a Mesozoic age. Comparison of tectonic and magnetic features on the seafloor with plate kinematic models shows that it is likely to have accreted to a mid-ocean ridge between the South American and Antarctic plates following their separation in Jurassic times. Subsequent regional shallowing may be related GJI Geodynamics and tectonics to subduction-related processes that preceded backarc extension in the East Scotia Sea. The presence of a fragment of Jurassic–Cretaceous ocean floor in the gateway implies that deep water connections through the Scotia Sea basin complex may have been possible since Eocene times when the continental tips of South America and the Antarctic Peninsula first passed each other. Key words: Tectonics and climate interactions; Kinematics of crustal and mantle deforma- tion; Antarctica; South America.