Scotia Arc: an Introduction
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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]. -
Marie Tharp: Mapping the Seafloor of Back-Arc Basins, Mid-Ocean Ridges, Continental Margins & Plate Boundaries Vienna (Austria), EGU 2020-3676, 7/5/2020
A Tribute to Marie Tharp: Mapping the seafloor of back-arc basins, mid-ocean ridges, continental margins & plate boundaries Vienna (Austria), EGU 2020-3676, 7/5/2020 Eulàlia Gràcia, Sara Martínez Loriente, Susana Diez, Laura Gómez de la Peña*, Cristina S. Serra, Rafael Bartolome, Valentí Sallarès, Claudio Lo Iacono, Hector Perea**, Roger Urgeles, Ingo Grevemeyer* and Cesar R. Ranero B-CSI at Institut de Ciències del Mar – CSIC, Barcelona *GEOMAR, Kiel, Germany **Universidad Complutense de Madrid, Facultad de Geologia, Madrid 1 The first steps of Marie Tharp • Marie Tharp, July 30, 1920 (Ypsilanti, Michigan) – August 23, 2006 (Nyack, New York) was an American geologist & oceano- graphic cartographer who, in partnership with Bruce Heezen, created the first scientific map of the Atlantic Ocean floor. • Tharp's work revealed the detailed topography and multi-dimensional geographical landscape of the ocean bottom. • Her work revealed the presence of a continuous rift-valley along the axis Fig. 1. A young Marie in the field helping his father, William E. of the Mid- Atlantic Ridge, causing a Tharp, a soil surveyor for United States Dpt. of Agriculture. Marie often paradigm shift in Earth Sciences that helped him with this task, which gave her an introduction to map- led to acceptance of Plate Tectonics making. From book “Soundings” by Hali Felt (2012). and Continental Drift. 2 Working at Columbia University Lamont Geological Observatory (NY) Fig. 2. Marie Fig. 3. at streets of Bruce New York, Heezen after she looking at a was hired to fathogram work by Dr. being Maurice produced by Ewing’, at an early the newly- echosounder formed (year 1940). -
Geodetic Determination of Relative Plate Motion and Crustal Deformation Across the Scotia-South America Plate Boundary in Eastern Tierra Del Fuego
Article Geochemistry 3 Volume 4, Number 9 Geophysics 19 September 2003 1070, doi:10.1029/2002GC000446 GeosystemsG G ISSN: 1525-2027 AN ELECTRONIC JOURNAL OF THE EARTH SCIENCES Published by AGU and the Geochemical Society Geodetic determination of relative plate motion and crustal deformation across the Scotia-South America plate boundary in eastern Tierra del Fuego R. Smalley, Jr. Center for Earthquake Research and Information, University of Memphis, 3876 Central Avenue, Ste. 1, Memphis, Tennessee 38152, USA ([email protected]) E. Kendrick and M. G. Bevis School of Ocean, Earth and Space Technology, University of Hawaii, 1680 East West Road, Honolulu, Hawaii 96822, USA ([email protected]; [email protected]) I. W. D. Dalziel and F. Taylor Institute of Geophysics, Jackson School of Geosciences, University of Texas at Austin, 4412 Spicewood Springs Road, Building 600, Austin, Texas 78759, USA ([email protected]; [email protected]) E. Laurı´a Instituto Geogra´fico Militar de Argentina, Cabildo 381, 1426 Buenos Aires, Argentina ([email protected]) R. Barriga Instituto Geogra´fico Militar de Chile, Nueva Santa Isabel 1640, Santiago, Chile ([email protected]) G. Casassa Centro de Estudios Cientı´ficos, Avda. Arturo Prat 514, Casilla 1469, Valdivia, Chile ([email protected]) E. Olivero and E. Piana Centro Austral de Investigaciones Cientı´ficas, Av. Malvinas Argentinas s/n, Caja de Correo 92, 9410 Ushuaia, Tierra del Fuego, Argentina ([email protected]; [email protected]) [1] Global Positioning System (GPS) measurements provide the first direct measurement of plate motion and crustal deformation across the Scotia-South America transform plate boundary in Tierra del Fuego. -
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. -
Geologic History of Siletzia, a Large Igneous Province in the Oregon And
Geologic history of Siletzia, a large igneous province in the Oregon and Washington Coast Range: Correlation to the geomagnetic polarity time scale and implications for a long-lived Yellowstone hotspot Wells, R., Bukry, D., Friedman, R., Pyle, D., Duncan, R., Haeussler, P., & Wooden, J. (2014). Geologic history of Siletzia, a large igneous province in the Oregon and Washington Coast Range: Correlation to the geomagnetic polarity time scale and implications for a long-lived Yellowstone hotspot. Geosphere, 10 (4), 692-719. doi:10.1130/GES01018.1 10.1130/GES01018.1 Geological Society of America Version of Record http://cdss.library.oregonstate.edu/sa-termsofuse Downloaded from geosphere.gsapubs.org on September 10, 2014 Geologic history of Siletzia, a large igneous province in the Oregon and Washington Coast Range: Correlation to the geomagnetic polarity time scale and implications for a long-lived Yellowstone hotspot Ray Wells1, David Bukry1, Richard Friedman2, Doug Pyle3, Robert Duncan4, Peter Haeussler5, and Joe Wooden6 1U.S. Geological Survey, 345 Middlefi eld Road, Menlo Park, California 94025-3561, USA 2Pacifi c Centre for Isotopic and Geochemical Research, Department of Earth, Ocean and Atmospheric Sciences, 6339 Stores Road, University of British Columbia, Vancouver, BC V6T 1Z4, Canada 3Department of Geology and Geophysics, University of Hawaii at Manoa, 1680 East West Road, Honolulu, Hawaii 96822, USA 4College of Earth, Ocean, and Atmospheric Sciences, Oregon State University, 104 CEOAS Administration Building, Corvallis, Oregon 97331-5503, USA 5U.S. Geological Survey, 4210 University Drive, Anchorage, Alaska 99508-4626, USA 6School of Earth Sciences, Stanford University, 397 Panama Mall Mitchell Building 101, Stanford, California 94305-2210, USA ABSTRACT frames, the Yellowstone hotspot (YHS) is on southern Vancouver Island (Canada) to Rose- or near an inferred northeast-striking Kula- burg, Oregon (Fig. -
Fate of the Cenozoic Farallon Slab from a Comparison of Kinematic Thermal Modeling with Tomographic Images
Earth and Planetary Science Letters 204 (2002) 17^32 www.elsevier.com/locate/epsl Fate of the Cenozoic Farallon slab from a comparison of kinematic thermal modeling with tomographic images Christian Schmid Ã, Saskia Goes, Suzan van der Lee, Domenico Giardini Institute of Geophysics, ETH Ho«nggerberg (HPP), 8093 Zu«rich, Switzerland Received 28May 2002; received in revised form 11 September 2002; accepted 18September 2002 Abstract After more than 100 million years of subduction, only small parts of the Farallon plate are still subducting below western North America today. Due to the relatively young age of the most recently subducted parts of the Farallon plate and their high rates of subduction, the subducted lithosphere might be expected to have mostly thermally equilibrated with the surrounding North American mantle. However, images from seismic tomography show positive seismic velocity anomalies, which have been attributed to this subduction, in both the upper and lower mantle beneath North America. We use a three-dimensional kinematic thermal model based on the Cenozoic plate tectonic history to quantify the thermal structure of the subducted Farallon plate in the upper mantle and determine which part of the plate is imaged by seismic tomography. We find that the subducted Farallon lithosphere is not yet thermally equilibrated and that its thermal signature for each time of subduction is found to be presently detectable as positive seismic velocity anomalies by tomography. However, the spatially integrated positive seismic velocity anomalies in tomography exceed the values obtained from the thermal model for a rigid, continuous slab by a factor of 1.5 to 2.0. -
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. -
West Antarctica: Tectonics and Paleogeography
Chapter 2 West Antarctica: Tectonics and Paleogeography The origin of West Antarctica (WANT) can be traced back to the Terra Australis orogenesis that began between 520 Ma and 510 Ma—shortly after the terminal suturing of Gondwana (Boger 2011). The onset of this event was responsible for the termination of passive margin sedimentation along much of the Pacific margin of Gondwana and marks the beginning of widespread and broadly coeval deforma- tion and arc-type plutonism. It also began a long-lived process of accretion that added much of the crust that defines eastern Australia, West Antarctica (domain 5 of Boger 2011, Fig. 2.1), and western South America (Cawood 2005, 2009). Post-Gondwana accretionary growth—the Terra Australis and Gondwanide Orogenies—The suturing of the West Gondwana and Australo–Antarctic plates along the Kuunga Orogen brought to an end the long-lived process of convergence between the pre-collision components of Gondwana. The result was a reconfigura- tion of the early to middle Cambrian plate system and the consequent transfer of ocean floor consumption from between the pre-Gondwana cratons to the outboard Pacific margin of newly formed Gondwana supercontinent (Cawood2005 ). This led to the establishment of the accretionary Terra Austrais Orogen (Cawood 2005), a general name given to the orogenic belt that stretched continuously from north- ern South America to northern Australia and which began in the early to middle Cambrian and lasted until the late Carboniferous. In Antarctica Terra Australis (Ross) orogenesis also deformed and variably metamorphosed the pre-Gondwana passive margin (Fig. 2.2). The Gondwana supercontinent underwent a sequential fragmentation over approximately 165 Ma. -
The Reception and Commemoration of William Speirs Bruce Are, I Suggest, Part
The University of Edinburgh School of Geosciences Institute of Geography A SCOT OF THE ANTARCTIC: THE RECEPTION AND COMMEMORATION OF WILLIAM SPEIRS BRUCE M.Sc. by Research in Geography Innes M. Keighren 12 September 2003 Declaration of originality I hereby declare that this dissertation has been composed by me and is based on my own work. 12 September 2003 ii Abstract 2002–2004 marks the centenary of the Scottish National Antarctic Expedition. Led by the Scots naturalist and oceanographer William Speirs Bruce (1867–1921), the Expedition, a two-year exploration of the Weddell Sea, was an exercise in scientific accumulation, rather than territorial acquisition. Distinct in its focus from that of other expeditions undertaken during the ‘Heroic Age’ of polar exploration, the Scottish National Antarctic Expedition, and Bruce in particular, were subject to a distinct press interpretation. From an examination of contemporary newspaper reports, this thesis traces the popular reception of Bruce—revealing how geographies of reporting and of reading engendered locally particular understandings of him. Inspired, too, by recent work in the history of science outlining the constitutive significance of place, this study considers the influence of certain important spaces—venues of collection, analysis, and display—on the conception, communication, and reception of Bruce’s polar knowledge. Finally, from the perspective afforded by the centenary of his Scottish National Antarctic Expedition, this paper illustrates how space and place have conspired, also, to direct Bruce’s ‘commemorative trajectory’—to define the ways in which, and by whom, Bruce has been remembered since his death. iii Acknowledgements For their advice, assistance, and encouragement during the research and writing of this thesis I should like to thank Michael Bolik (University of Dundee); Margaret Deacon (Southampton Oceanography Centre); Graham Durant (Hunterian Museum); Narve Fulsås (University of Tromsø); Stanley K. -
Driving the Upper Plate Surface Deformation by Slab Rollback and Mantle Flow Pietro Sternai, Laurent Jolivet, Armel Menant, Taras Gerya
Driving the upper plate surface deformation by slab rollback and mantle flow Pietro Sternai, Laurent Jolivet, Armel Menant, Taras Gerya To cite this version: Pietro Sternai, Laurent Jolivet, Armel Menant, Taras Gerya. Driving the upper plate surface defor- mation by slab rollback and mantle flow. Earth and Planetary Science Letters, Elsevier, 2014, 405, pp.110-118. 10.1016/j.epsl.2014.08.023. insu-01064803 HAL Id: insu-01064803 https://hal-insu.archives-ouvertes.fr/insu-01064803 Submitted on 17 Sep 2014 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Driving the upper plate surface deformation by slab rollback and mantle flow Pietro Sternai*1, Laurent Jolivet1, Armel Menant1 and Taras Gerya2 1 Institut de Sciences de la Terre d’Orléans (ISTO) - University of Orléans, France 2 Institute of Geophysics - Swiss Federal Institute of Technology (ETH), Zürich, Switzerland *Correspondence to: [email protected] The relative contribution of crustal and mantle processes to surface deformation at convergent plate margins is still controversial. Conflicting models involving either extrusion mechanisms or slab rollback, in particular, were proposed to explain the surface strain and kinematics across the Tethyan convergent domain. -
Gjoa Haven © Nunavut Tourism
NUNAVUT COASTAL RESOURCE INVENTORY ᐊᕙᑎᓕᕆᔨᒃᑯᑦ Department of Environment Avatiliqiyikkut Ministère de l’Environnement Gjoa Haven © Nunavut Tourism ᐊᕙᑎᓕᕆᔨᒃᑯᑦ Department of Environment Avatiliqiyikkut NUNAVUT COASTAL RESOURCE INVENTORY • Gjoa Haven INVENTORY RESOURCE COASTAL NUNAVUT Ministère de l’Environnement Nunavut Coastal Resource Inventory – Gjoa Haven 2011 Department of Environment Fisheries and Sealing Division Box 1000 Station 1310 Iqaluit, Nunavut, X0A 0H0 GJOA HAVEN Inventory deliverables include: EXECUTIVE SUMMARY • A final report summarizing all of the activities This report is derived from the Hamlet of Gjoa Haven undertaken as part of this project; and represents one component of the Nunavut Coastal Resource Inventory (NCRI). “Coastal inventory”, as used • Provision of the coastal resource inventory in a GIS here, refers to the collection of information on coastal database; resources and activities gained from community interviews, research, reports, maps, and other resources. This data is • Large-format resource inventory maps for the Hamlet presented in a series of maps. of Gjoa Haven, Nunavut; and Coastal resource inventories have been conducted in • Key recommendations on both the use of this study as many jurisdictions throughout Canada, notably along the well as future initiatives. Atlantic and Pacific coasts. These inventories have been used as a means of gathering reliable information on During the course of this project, Gjoa Haven was visited on coastal resources to facilitate their strategic assessment, two occasions: