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The Structure and Transport of the Agulhas Return Current
The Structure and Transport of the Agulhas Return Current Isabelle Jane Ansorge Submitted in fulfillment of the requirements of the Master of Science degree Department of Oceanography University of Cape Town 1996 University of Cape Town The copyright of this thesis vests in the author. No quotation from it or information derived from it is to be published without full acknowledgement of the source. The thesis is to be used for private study or non- commercial research purposes only. Published by the University of Cape Town (UCT) in terms of the non-exclusive license granted to UCT by the author. University of Cape Town I ABSTRACT The Agulhas Current flows along the eastern coast of southern Africa as one of the largest western boundary currents in the world's ocean. On overshooting the southern tip of Africa at approximately 20°E, a retroflection loop is formed that causes the current to double back on itself and to fonn the easterly flowing Agulhas Return Current. No focussed investigation to establish the hydrography of this imponant component of global ocean circulation has to date been carried out. To trace the Agulhas Return Current's passage eastwards into the South Indian Ocean, data collected from six CTD hydrographic cruises; AJAX, ARC, SCARC, Marathon, Discovery 164 and SUZIL, as well as from three XBT temperature cruises,· Marion 83, Gallieni 72 and FIBEX, have been analysed. It is shown that the Agulhas Return Current initially flows zonally from 20°-25°E at a latitude approximately 39°30'-40°30'S before forming a planetary wave over the Agulhas Plateau between 25°-28°E. -
Joint Geological Survey/University of Cape Town MARINE GEOSCIENCE UNIT TECHNICAL ^REPORT NO. 13 PROGRESS REPORTS for the YEARS 1
Joint Geological Survey/University of Cape Town MARINE GEOSCIENCE UNIT TECHNICAL ^REPORT NO. 13 PROGRESS REPORTS FOR THE YEARS 1981-1982 Marine Geoscience Group Department of Geology University of Cape Town December 1982 NGU-Tfc—Kh JOINT GEOLOGICAL SURVEY/UNIVERSITY OF CAPE TOWN MARINE GEOSCIENCE UNIT TECHNICAL REPORT NO. 13 PROGRESS REPORTS FOR THE YEARS 1981-1982 Marine Geoscience Group Department of Geology University of Cape Town December 1982 The Joint Geological Survey/University of Cape Town Marine Geoscience Unit is jointly funded by the two parent organizations to promote marine geoscientific activity in South Africa. The Geological Survey Director, Mr L.N.J. Engelbrecht, and the University Research Committee are thanked for their continued generous financial and technical support for this work. The Unit was established in 1975 by the amalgamation of the Marine Geology Programme (funded by SANCOR until 1972) and the Marine Geophysical Unit. Financial ?nd technical assistance from the South African National Committee for Oceanographic Research, and the National Research Institute for Oceanology (Stellenbosch) are also gratefully acknowledged. It is the policy of the Geological Survey and the University of Cape Town that the data obtained may be presented in the form of theses for higher degrees and that completed projects shall be published without delay in appropriate media. The data and conclusions contained in this report are made available for the information of the international scientific community with tl~e request that they be not published in any manner without written permission. CONTENTS Page INTRODUCTION by R.V.Dingle i PRELIMINARY REPORT ON THE BATHYMETRY OF PART OF 1 THE TRANSKEI BASIN by S.H. -
Connecting the Deep Earth and the Atmosphere
In Mantle Convection and Surface Expression (Cottaar, S. et al., eds.) AGU Monograph 2020 (in press) Connecting the Deep Earth and the Atmosphere Trond H. Torsvik1,2, Henrik H. Svensen1, Bernhard Steinberger3,1, Dana L. Royer4, Dougal A. Jerram1,5,6, Morgan T. Jones1 & Mathew Domeier1 1Centre for Earth Evolution and Dynamics (CEED), University of Oslo, 0315 Oslo, Norway; 2School of Geosciences, University of Witwatersrand, Johannesburg 2050, South Africa; 3Helmholtz Centre Potsdam, GFZ, Telegrafenberg, 14473 Potsdam, Germany; 4Department of Earth and Environmental Sciences, Wesleyan University, Middletown, Connecticut 06459, USA; 5DougalEARTH Ltd.1, Solihull, UK; 6Visiting Fellow, Earth, Environmental and Biological Sciences, Queensland University of Technology, Brisbane, Queensland, Australia. Abstract Most hotspots, kimberlites, and large igneous provinces (LIPs) are sourced by plumes that rise from the margins of two large low shear-wave velocity provinces in the lowermost mantle. These thermochemical provinces have likely been quasi-stable for hundreds of millions, perhaps billions of years, and plume heads rise through the mantle in about 30 Myr or less. LIPs provide a direct link between the deep Earth and the atmosphere but environmental consequences depend on both their volumes and the composition of the crustal rocks they are emplaced through. LIP activity can alter the plate tectonic setting by creating and modifying plate boundaries and hence changing the paleogeography and its long-term forcing on climate. Extensive blankets of LIP-lava on the Earth’s surface can also enhance silicate weathering and potentially lead to CO2 drawdown (cooling), but we find no clear relationship between LIPs and post-emplacement variation in atmospheric CO2 proxies on very long (>10 Myrs) time- scales. -
Gondwana Breakup Via Double-Saloon-Door Rifting and Seafloor Spreading in a Backarc Basin During Subduction Rollback
Available online at www.sciencedirect.com Tectonophysics 445 (2007) 245–272 www.elsevier.com/locate/tecto Gondwana breakup via double-saloon-door rifting and seafloor spreading in a backarc basin during subduction rollback A.K. Martin Repsol YPF Exploración, Al Fattan Plaza, PO Box 35700, Dubai, United Arab Emirates Received 2 February 2007; received in revised form 4 July 2007; accepted 21 August 2007 Available online 28 August 2007 Abstract A model has been developed where two arc-parallel rifts propagate in opposite directions from an initial central location during backarc seafloor spreading and subduction rollback. The resultant geometry causes pairs of terranes to simultaneously rotate clockwise and counterclockwise like the motion of double-saloon-doors about their hinges. As movement proceeds and the two terranes rotate, a gap begins to extend between them, where a third rift initiates and propagates in the opposite direction to subduction rollback. Observations from the Oligocene to Recent Western Mediterranean, the Miocene to Recent Carpathians, the Miocene to Recent Aegean and the Oligocene to Recent Caribbean point to a two-stage process. Initially, pairs of terranes comprising a pre-existing retro-arc fold thrust belt and magmatic arc rotate about poles and accrete to adjacent continents. Terrane docking reduces the width of the subduction zone, leading to a second phase during which subduction to strike-slip transitions initiate. The clockwise rotated terrane is caught up in a dextral strike-slip zone, whereas the counterclockwise rotated terrane is entrained in a sinistral strike-slip fault system. The likely driving force is a pair of rotational torques caused by slab sinking and rollback of a curved subduction hingeline. -
International Ocean Discovery Program Expedition 361 Preliminary Report South African Climates (Agulhas LGM Density Profile)
International Ocean Discovery Program Expedition 361 Preliminary Report South African Climates (Agulhas LGM Density Profile) 30 January–31 March 2016 Ian R. Hall, Sidney R. Hemming, Leah J. LeVay, and the Expedition 361 Scientists Publisher’s notes Core samples and the wider set of data from the science program covered in this report are under moratorium and accessible only to Science Party members until 30 September 2017. This publication was prepared by the JOIDES Resolution Science Operator (JRSO) at Texas A&M University (TAMU) as an account of work performed under the International Ocean Discovery Pro- gram (IODP). Funding for IODP is provided by the following international partners: National Science Foundation (NSF), United States Ministry of Education, Culture, Sports, Science and Technology (MEXT), Japan European Consortium for Ocean Research Drilling (ECORD) Ministry of Science and Technology (MOST), People’s Republic of China Korea Institute of Geoscience and Mineral Resources (KIGAM) Australia-New Zealand IODP Consortium (ANZIC) Ministry of Earth Sciences (MoES), India Coordination for Improvement of Higher Education Personnel, Brazil (CAPES) Portions of this work may have been published in whole or in part in other International Ocean Discovery Program documents or publications. Disclaimer Any opinions, findings, and conclusions or recommendations expressed in this publication are those of the author(s) and do not necessarily reflect the views of the participating agencies, TAMU, or Texas A&M Research Foundation. Copyright Except where otherwise noted, this work is licensed under a Creative Commons Attribution License. Unrestricted use, distribution, and reproduction is permitted, provided the original author and source are credited. Citation Hall, I.R., Hemming, S.R., LeVay, L.J., and the Expedition 361 Scientists, 2016. -
JOIDES Resolution Expedition 361 (Southern African Climates) Site
IODP Expedition 361: Southern African Climates Site U1475 Summary Background and Objectives Site U1475 is located on the southwestern flank of Agulhas Plateau (41°25.61′S, 25°15.64′E), ~450 nmi south of Port Elizabeth, South Africa, in a water depth of 2669 mbsl. The Agulhas Plateau, which was formed during the early stages of the opening of the South Atlantic about 90 Ma (Parsiegla et al., 2008), is a major bathymetric high that is variably coated with sediments (Uenzelmann Neben, 2001). The 230,000 km2 plateau, which ascends up to ~2500 m above the adjacent seafloor, is bounded on the north by the 4700 m deep Agulhas Passage and is flanked by the Agulhas Basin in the west and the Transkei Basin in the northeast. The northern part of the plateau is characterized by rugged topography, while the central and southern part of the plateau exhibits a relatively smooth topography (Allen and Tucholke, 1981) and has greater sediment thickness (Uenzelmann Neben, 2001). A strong water mass transport flows across the Agulhas Plateau region (Macdonald, 1993), which involves the water column from the surface down to Upper Circumpolar Deep Water. The hydrography of the upper ocean is dominated by the Agulhas Return Current, which comprises the component of the Agulhas Current that is not leaked to the South Atlantic Ocean but rather flows eastwards from the retroflection (Lutjeharms and Ansorge, 2001). Antarctic Intermediate Water, below the Agulhas Return Current, also follows the same flow path near South Africa as the Agulhas Current showing a similar retroflection (Lutjeharms, 1996). -
The Shatsky Rise Oceanic Plateau Structure from Two-Dimensional Multichannel Seismic Refl Ection Profi Les and Implications for Oceanic Plateau Formation
Downloaded from specialpapers.gsapubs.org on June 2, 2015 The Geological Society of America Special Paper 511 2015 The Shatsky Rise oceanic plateau structure from two-dimensional multichannel seismic refl ection profi les and implications for oceanic plateau formation Jinchang Zhang* William W. Sager† Department of Oceanography, Texas A&M University, College Station, Texas 77843, USA Jun Korenaga Department of Geology and Geophysics, Yale University, New Haven, Connecticut 06520, USA ABSTRACT The Shatsky Rise is one of the largest oceanic plateaus, a class of volcanic fea- tures whose formation is poorly understood. It is also a plateau that was formed near spreading ridges, but the connection between the two features is unclear. The geologic structure of the Shatsky Rise can help us understand its formation. Deeply penetrating two-dimensional (2-D) multichannel seismic (MCS) refl ection profi les were acquired over the southern half of the Shatsky Rise, and these data allow us to image its upper crustal structure with unprecedented detail. Synthetic seismo- grams constructed from core and log data from scientifi c drilling sites crossed by the MCS lines establish the seismic response to the geology. High-amplitude basement refl ections result from the transition between sediment and underlying igneous rock. Intrabasement refl ections are caused by alternations of lava fl ow packages with dif- fering properties and by thick interfl ow sediment layers. MCS profi les show that two of the volcanic massifs within the Shatsky Rise are immense central volcanoes. The Tamu Massif, the largest (~450 km × 650 km) and oldest (ca. 145 Ma) volcano, is a single central volcano with a rounded shape and shallow fl ank slopes (<0.5°–1.5°), characterized by lava fl ows emanating from the volcano center and extending hun- dreds of kilometers down smooth, shallow fl anks to the surrounding seafl oor. -
Tectonic History, Microtopography and Bottom Water Circulation of the Natal Valley and Mozambique Ridge, Southwest Indian Ocean
Tectonic history, microtopography and bottom water circulation of the Natal Valley and Mozambique Ridge, southwest Indian Ocean. By: Errol Avern Wiles Submitted in fulfilment of the degree Doctor of Philosophy In the Discipline of Geological Sciences School of Agricultural, Earth and Environmental Sciences College of Agriculture, Engineering and Science University of KwaZulu Natal, Durban South Africa 2014 i Preface The experimental work described in this thesis was carried out in the Discipline of Geological Sciences, University of KwaZulu-Natal, Westville, from July 2010 to November 2014, under the supervision of Prof. Watkeys, Dr. Green and Prof. Jokat. These studies represent original work by the author and have not otherwise been submitted in any form for any degree or diploma to any tertiary institution. Where use has been made of the work of others it is duly acknowledged in the text. Signed:_____________________ Name:________________________ Date:_____________ ii Declaration 1 – Plagiarism I, Errol Avern Wiles, declare that: 1. The research reported in this thesis, except where otherwise indicated, is my original research. 2. This thesis has not been submitted for any degree or examination at any other university. 3. This thesis does not contain other persons’ data, graphs or other information, unless specifically acknowledged as being sourced from other persons. 4. This thesis does not contain any other persons writing, unless specifically acknowledged as being sourced from other researchers. Where other written sources have been quoted then: a. Their words have been re-written but the general information attributed to them has been referenced b. Where their exact words have been used, then their writing has been placed in italics and inside quotation marks, and referenced. -
Deep Sea Drilling Project Initial Reports Volume 26
INDEX Africa Antarctica, separation, 918 Bottom water, 937 Agulhas Plateau, 949 Boundaries, criteria used to locate, 678 Albian foraminifera assemblages, 750 Boundary, biostratigraphic, 677 Albian-Cenomanian foraminifera, 747 foraminifera, Amphipyndax enesseffi Zone, 774 Miocene/Pliocene, 678 Amsterdam-St. Paul volcanic complex, 924 Oligocene/Miocene, 678 Angiosperms, 816 Pleistocene/Holocene, 680 Angular unconformity, 283, 288 Pliocene/Miocene, 687 Antarctic Bottom Water, 918 Pliocene/Quaternary, 679 Antarctica, separation of Africa, 918 Quaternary/Pliocene, 677, 687 Argon, nonradiogenic, 514 Brachiopod, 167 Argon analyses, 513 Broken Ridge, 8, 9, 233, 243, 281, 288, 359, 370, 418, Artostrobiom urna Zone, 772, 774, 775 925, 950 Aseismic ridges, 571, 910 Broken Ridge-Naturaliste Plateau, 7 Australian continental margin, 419 Bryozoans, 166, 167 Australian plate, 233 Calcareous nannoplankton, Site 251, 84 Authigenic garnet, 80, 85, 593, 594, 915 Calcispheres, 335, 747 Basalt, 80, 161, 162, 238, 301, 329, 331, 336, 466 Campanian-lower Eocene unconformity, 619 classification of tholeiites, 480 Carbon emmission spectrography, 541 criteria for recognizing altered, 472 Carbon-carbonate analysis, 16 crystallization differentiation, 481 Carbonate compensation depth, 140, 306, 336, 419, 950 electrical resistivity of, 505 Carlsberg Ridge, Central Indian Ridge, spreading on, grain-size range, 533 913 hematite in, 533 Celadonite,471 normative compositions, 477 Cenozoic species, nannoplankton, 619 ocean ridge, 484 Central Indian Basin, 418 olivine, -
Geochemistry, Geophysics, Geosystems
Geochemistry, Geophysics, Geosystems RESEARCH ARTICLE The Strike-Slip West Wishbone Ridge and the Eastern Margin of 10.1002/2017GC007372 the Hikurangi Plateau Key Points: R. S. Barrett1,2 , B. Davy3 , T. Stern1 , and K. Gohl4 The West Wishbone Ridge is recognized as having been a dextral 1Victoria University of Wellington, Institute of Geophysics, Wellington, New Zealand, 2Now at Christian-Albrechts- strike-slip fault during the Cretaceous University of Kiel, Institute of Geophysics, Kiel, Germany, 3GNS Science, Avalon, Lower Hutt, New Zealand, 4Department of The present-day eastern margin of the Hikurangi Plateau between Geosciences, Alfred Wegener Institute Helmholtz-Center for Polar and Marine Research, Bremerhaven, Germany 42-438S is located using seismic reflection data and gravity modeling We identify over-thickened oceanic Abstract The West Wishbone Ridge (WWR), east of New Zealand, has previously been interpreted as a crust north of, and proximal to the Cretaceous plate boundary, although both the nature and timing of motion along this feature have been Hikurangi Plateau disputed. Here, using recently acquired seismic reflection data from the region of the intersection of the WWR with the Chatham Rise, we show that the WWR was primarily a dextral strike-slip fault during the Late Correspondence to: R. Barrett, Cretaceous. The WWR first propagated along the eastern margin of the Hikurangi Plateau after the collision [email protected] of the Hikurangi Plateau with the Chatham Rise, in response to the slowing of spreading at the Osbourn Trough while spreading continued unabated east of the East Wishbone Ridge, from ca. 105 Ma. Reorienta- Citation: tion of spreading at the Osbourn Trough at this time resulted in short-lived, oblique subduction beneath Barrett, R. -
Washington, DC 20546
46 Final. Report IMPROVING THE GEOLGICAL 1"'ERPRE"IATION OF IGGNETIC AND GRAVITY SATELTiITE ANOI'IALIES (4/1/85 - 11/31/86) Grant No. NAW-736 (Basic) submitted to Eational Aeronautics & Space Administration Code EE1 NASA Headquarters .Washington, DC 20546 January, 1987 (NASA-CR- 180 149) IMPEDVING ?kE GEOLOGICAL Nd7- 154 18 .Ih!IEEEBE'IATION OF EAGbETIC ABC GhAVXTY SAZELLIIE ANGEALIES Final 3e~crt,1 Apr. 1585 - 31 Nov, 19k6 (Furdue Uriv-) 124 p Unclds CSCL 086 G3/46 437b3 William J. Hinze and Lawrence W. Braile Ralph R.B. von Frese Department of Earth & De*. of Geology & Atmospheric Sciences Mine ralogy Purdue University Ohio State University West Lafayette, IN 47907 Columbus, OH 43210 IFIPIMVIIG THE GEOLGICAL INTERPRFTATION OF MIy;NETIC AND GRAVITY SATELLITE A"&IES Abstract Quantitative analysis of the geologic component of observed satellite magnetic and gravity fields requires accurate isolation of the geologic component of the observations, theoretically sound and viable inversion techniques, and integration of collateral, constraining geologic and geophysical data. A number of significant contributions have been made in this study which make quantitative analysis more accurate. These include procedures for 1) screening and processing orbital data for lithospheric signals based on signal repeatability and wavelength analysis; 2) producing accurate gridded anormly values at constant elevations from the orbital data by three-dimensional least squares collocation; 3) increasing the stability of equivalent point source inversion and criteria for the selection of the optimum wing parameter; 4) enhancing inversion techniques through an iterative procedure based on the superposition theorem of potential fields; and 5) modeling efficiently regional-scale lithospheric sources of satellite magnetic anomalies. -
Aalenian, 661, 687 Abu Swayel, 208 Abyssal Fan, 562 Acoustic
INDEX Aalenian, 661, 687 Algal-Oolitic limestones, 171 Abu Swayel, 208 Alkali basalt, 71, 77, 79, 220, 229, 605 Abyssal fan, 562 Alkali-Olivine basalt, 79, 232, 241, 613, Acoustic basement, 73, 75, 81, 406, 408 623, 625 Acritarchs, 159 Alkaline trachyte, 209 Adamellites, 590 Alpine diastrophism, 241-242, 244-245 Adelaide Geosyncline, 547-548 Alula-Fartak Trench, 87 Adelaidean Belt, 742 Aluvial fans, 154 Aden, 271, 358 Amarante Passage, 26 Aden Volcanic Series, 220, 267, 271, 278 Amba Aradam Formation, 218 Adigrat Sandstone, 273-274 Ambokahave Shales, 677 Aeclian deposits, 161 America-Antarctica Ridge, 97 Aeolan sand, 548 Amery Ice Shelf, 702, 705-707, 730 Aeromagnetic surveys, 554, 726 Amiran Flysch, 326 Afanasy Nikitin Seamount, 77 Amirante Island, 591 Afar Depression, 88 Amirante Ridge, 591 Afar Rift Zone, 87 Amirante Trench, 117 Afar Series, 279 Amirantes, 129 Afar Triangle, 288 Ammonia beccarrii. 382 Africa, 31 Ammonites, 166, 169, 188, 519, 659-660, African-Antarctic Basin, 54, 77, 86, 136 676,692 Agulhas Bank, 73 Ammonoids, 517-518 Agulhas Basin, 54, 74 Ampandrandava Group, 652 Agulhas Current, 6, 28 Ampasimena Series, 661 Agulhas Fracture Zone, 74, 164 Amphibians, 160,659 Agulhas Plateau, 6, 15, 52, 73-74 Amphibolites, 208, 333, 455, 653, 709, 721, Albany-Fraser Mobile Zone, 527 723-729, 735-736 Albany-Fraser Province, 740, 742 Amphistegina. 606 Albian, 82, 127-128, 165, 189,406,664, Amsterdam Fracture Zone, 631 677, 679, 690 Amsterdam Island, 631-632 Alcock Seamount, 422, 424, 427 Anahita Fracture Zone, 91 Algae, 606 Andaman Island,