Deep Sea Drilling Project Initial Reports Volume 26
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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. -
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. -
This Article Appeared in a Journal Published by Elsevier. the Attached
This article appeared in a journal published by Elsevier. The attached copy is furnished to the author for internal non-commercial research and education use, including for instruction at the authors institution and sharing with colleagues. Other uses, including reproduction and distribution, or selling or licensing copies, or posting to personal, institutional or third party websites are prohibited. In most cases authors are permitted to post their version of the article (e.g. in Word or Tex form) to their personal website or institutional repository. Authors requiring further information regarding Elsevier’s archiving and manuscript policies are encouraged to visit: http://www.elsevier.com/copyright Author's personal copy Marine Geology 266 (2009) 65–79 Contents lists available at ScienceDirect Marine Geology journal homepage: www.elsevier.com/locate/margeo Sedimentary deposits on the southern South African continental margin: Slumping versus non-deposition or erosion by oceanic currents? Gabriele Uenzelmann-Neben a,⁎, Katrin Huhn b a Alfred-Wegener-Institut für Polar- und Meeresforschung, Am Alten Hafen 26, 27572 Bremerhaven, Germany b MARUM, Center for Marine Environmental Sciences, University of Bremen, Leobener Str., 28359 Bremen, Germany article info abstract Article history: Seismic profiles extending from the southern South African shelf into the deep sea reveal a strong erosional Received 5 January 2009 activity, which affects large parts of the continental margin. Quaternary to Oligocene units and, in places, the Received in revised form 15 July 2009 complete sedimentary column appear to have been removed. Mass movements were previously considered Accepted 17 July 2009 as the origin of this erosion. However, structures indicating slumping can be identified in only a few places. -
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, -
Gondwana Breakup: Messages from the North Natal Valley M
Gondwana breakup: messages from the North Natal Valley M. Moulin, D. Aslanian, M. Evain, A. Leprêtre, P. Schnürle, F. Verrier, J. Thompson, P. de Clarens, Sylvie Leroy, N. Dias, et al. To cite this version: M. Moulin, D. Aslanian, M. Evain, A. Leprêtre, P. Schnürle, et al.. Gondwana breakup: messages from the North Natal Valley. Terra Nova, Wiley-Blackwell, 2020, 32 (3), pp.205-214. 10.1111/TER.12448. hal-02429986 HAL Id: hal-02429986 https://hal.archives-ouvertes.fr/hal-02429986 Submitted on 20 Nov 2020 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. DR MARYLINE MOULIN (Orcid ID : 0000-0002-5685-2451) Article type : Paper Title of manuscript: Gondwana breakup: messages from the North Natal Valley M. Moulin1*, D. Aslanian1, M. Evain1, A. Leprêtre1,2, P. Schnurle1, F. Verrier1, J. Thompson1, P. De Clarens3, S. Leroy4, N. Dias5,6 and the PAMELA-MOZ35 Team1,2,3,4,5,6,7,8,9,10,11,12,13 1 Ifremer, REM/GM/LGS, Centre de Brest, 29280 Plouzané, France, [email protected] 2 LGO, Laboratoire Geosciences Ocean, IUEM, CNRS, 29280 Plouzané, France 3 Total, R&D, avenue Larribau, 64000 Pau, France 4 UPMC, Univ Paris 6, CNRS UMR 7193, ISTEP, 4 place Jussieu, 75005 Paris, France 5 ISEL - Instituto Superior de Engenharia de Lisboa, Lisboa, Portugal 6 IDL – Instituto Dom Luis, Lisboa, Faculdade das Ciências da Universidade de Lisboa, 1749-016 Lisboa, Portugal 7 AWI, Am Alten Hafen 26, D-27568 Bremerhaven, Germany 8 BGR, Geozentrum Hannover, Stilleweg 2, 30655 Hannover, Germany 9 INAMI, Praça 25 de Junho, n°380, P.O. -
Large Igneous Provinces and Silicic Large Igneous Provinces
Large igneous provinces and silicic large 1888 2013 igneous provinces: Progress in our understanding CELEBRATING ADVANCES IN GEOSCIENCE over the last 25 years Invited Review Scott E. Bryan1,† and Luca Ferrari2,3,† 1School of Earth, Environmental and Biological Sciences, Queensland University of Technology, GPO Box 2434, Brisbane, 4001, Australia 2Centro de Geociencias, Universidad Nacional Autonoma de Mexico, Boulevard Juriquilla 3001, Querétaro, 76230, Mexico 3Instituto de Geología, Universidad Nacional Autonoma de Mexico, Circuito Investigacion Cientifi ca, Ciudad Universitaria, Mexico City, 04510, Mexico ABSTRACT margins, where, in the latter setting, large ig- ities, and are characterized by igneous pulse(s) neous province magmatism can be dominated of short duration (1–5 m.y.), during which a Large igneous provinces are exceptional by silicic products. (3) Mineral and energy re- large proportion (>75%) of the total igneous intraplate igneous events throughout Earth’s sources, with major platinum group elements volume was emplaced (Bryan and Ernst, 2008). history. Their signifi cance and potential (PGEs) and precious metal resources, are Continental fl ood basalt provinces, such as the global impact are related to the total volume hosted in these provinces, as well as magma- Deccan Traps, Siberian Traps, and Columbia of magma intruded and released during these tism impacting on the hydro carbon potential River fl ood basalt province, are some of the best geologically brief events (peak eruptions are of volcanic basins and rifted margins through recognized examples of continental large igne- often within 1–5 m.y. in duration) where mil- enhancing source-rock maturation, providing ous provinces (Fig. 1). While continental fl ood lions to tens of millions of cubic kilometers fl uid migration pathways, and initiating trap basalt provinces had been widely recognized of magma are produced. -
Crustal Structure of the Southern Margin of the African Plate: Results
Originally published as: Stankiewicz, J., Parsiegla, N., Ryberg, T., Gohl, K, Weckmann, U., Trumbull, R., Weber, M. (2008): Crustal Structure of the Southern Margin of the African Continent: Results from Geophysical Experiments. - Journal of Geophysical Research, 113, B10313 DOI: 10.1029/2008JB005612. 1 Crustal Structure of the Southern Margin of the African 2 Continent: Results from Geophysical Experiments. 3 4 J. Stankiewicz, N. Parsiegla, T. Ryberg, K. Gohl, U. Weckmann, R. Trumbull & M. Weber. 5 6 Abstract 7 A number of geophysical onshore and offshore experiments were carried out along a profile across the 8 southern margin of the African Plate in the framework of the Inkaba yeAfrica project. Refraction 9 seismic experiments show that Moho depth decreases rapidly from over 40 km inland to around 30 km 10 at the present coast, before gently thinning out towards the Agulhas-Falkland Fracture Zone, which 11 marks the transition zone between continental and oceanic crust. In the region of the abruptly 12 decreasing Moho depth, in the vicinity of the boundary between the Namaqua-Natal Mobile Belt and 13 the Cape Fold Belt, lower crustal P-wave velocities up to 7.4 km/s are observed. This is interpreted as 14 metabasic lithologies of Precambrian age in the Namaqua-Natal Mobile Belt, or mafic intrusions added 15 to the base of the crust by younger magmatism. The velocity model for the upper crust has excellent 16 resolution, and is consistent with the known geological record. A joint interpretation of the velocity 17 model with an electrical conductivity model, obtained from magnetotelluric studies, makes it possible 18 to correlate a high velocity anomaly north of the centre of the Beattie Magnetic Anomaly with a highly 19 resistive body. -
The Agulhas Plateau: Structure and Evolution of a Large Igneous Province
Geophys. J. Int. (2008) 174, 336–350 doi: 10.1111/j.1365-246X.2008.03808.x The Agulhas Plateau: structure and evolution of a Large Igneous Province N. Parsiegla, K. Gohl and G. Uenzelmann-Neben Alfred Wegener Institute for Polar and Marine Research, PO Box 12161, 27515 Bremerhaven, Germany. E-mail: [email protected] Accepted 2008 March 28. Received 2008 March 13; in original form 2008 January 5 SUMMARY Large Igneous Provinces (LIP) are of great interest due to their role in crustal generation, magmatic processes and environmental impact. The Agulhas Plateau in the southwest Indian Ocean off South Africa has played a controversial role in this discussion due to unclear evidence for its continental or oceanic crustal affinity. With new geophysical data from seismic refraction and reflection profiling, we are able to present improved evidence for its crustal structure and composition. The velocity–depth model reveals a mean crustal thickness of 20 km with a maximum of 24 km, where three major units can be identified in the crust. In our seismic reflection records, evidence for volcanic flows on the Agulhas Plateau can be observed. The middle crust is thickened by magmatic intrusions. The up to 10 km thick lower crustal body is characterized by high seismic velocities of 7.0–7.6 km s−1. The velocity–depth distribution suggests that the plateau consists of overthickened oceanic crust similar to other oceanic LIPs such as the Ontong-Java Plateau or the northern Kerguelen Plateau. The total volume of the Agulhas Plateau was estimated to be 4 × 106 km3 of which about 10 per cent consists of extruded igneous material.