2,473 research outputs found

    Seismic characteristics of sediment drifts: An example from the Agulhas Plateau, southwest Indian Ocean

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    Sediment drifts provide information on the palaeoceanographic development of a region. Additionally, they may represent hydrocarbon reservoirs. Because of this, sediment drift investigation has increased over the last few years. Nevertheless, a number of problems remain regarding the processes controlling their shape, the characteristic lithological and seismic patterns and the diagnostic criteria.As an example, sediment drifts from the Agulhas Plateau, southwest Indian Ocean, are presented here. They show a variety of seismic features and facies including an asymmetric mounded geometry, changes in internal reflection pattern, truncation of internal reflectors at the seafloor and discontinuities. This collection of observations in combination with the local oceanography appears to comprise a diagnostic tool for sediment drifts

    The Agulhas Ridge, South Atlantic: the peculiar structure of a fracture zone

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    The Agulhas Ridge is a prominent topographic feature that parallels the Agulhas-Falkland Fracture Zone (AFFZ). Seismic reflection and wide angle/refraction data have led to the classification of this feature as a transverse ridge. Changes in spreading rate and direction associated with ridge jumps, combined with asymmetric spreading within the Agulhas Basin, modified the stress field across the fracture zone. Moreover, passing the Agulhas Ridges location between 80 Ma and 69 Ma, the Bouvet and Shona Hotspots may have supplied excess material to this part of the AFFZ thus altering the ridges structure.The low crustal velocities and overthickened crust of the northern Agulhas Ridge segment indicate a possible continental affinity that suggests it may be formed by a small continental sliver, which was severed off the Maurice Ewing Bank during the opening of the South Atlantic.In early Oligocene times the Agulhas Ridge was tectono-magmatically reactivated, as documented by the presence of basement highs disturbing and disrupting the sedimentary column in the Cape Basin. We consider the Discovery Hotspot, which distributes plume material southwards across the AAFZ, as a source for the magmatic material

    The structure and classification of the Mozambique Ridge based on seismic reflection data

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    The Mozambique Ridge (MozR), a prominent basement high in the southwestern Indian Ocean, consists of four major geomorphological units associated with numerous phases of volcanic activity between 140 Ma and 122 Ma. Over the last decades nature and origin of the Mozambique Ridge have been intensely debated with one hypothesis suggesting a Large Igneous Province (LIP) origin. This would have had immense influence on climate during the early Cretaceous with the emission of gases and heat into atmosphere and ocean but also implications on the development of the South African gateway with the formation of obstacles for surface and deep circulation. An extensive seismic survey was conducted over the Mozambique Ridge with the aim of solving the questions about its origin and evolution. High-resolution seismic reflection data reveals a number of magmatic centers with a random distribution. Intra-basement reflections can be identified up to several hundred ms TWT below top of basement. The internal reflections generally dip away from their magmatic centers and individual reflections can typically be traced for 5-15 km. These are interpreted to represent massive lava flow units, which are characteristic of oceanic plateau eruptions. Additionally to primary volcanic features associated with the initial emplacement of the individual segments of the Mozambique Ridge we identify secondary volcanic features indicating magmatic reactivation after its initial build-up. The total volume of the southern Mozambique Ridge is estimated to be 2.2 x 106 km3. We use this estimation to obtain a more precise reconstruction for the emplacement of the Mozambique Ridge. Based on our results we propose an oceanic LIP origin of the southern Mozambique Ridge and show that our data points toward a sequential development of its segments

    Effects of Antenna Beam Chromaticity on Redshifted 21~cm Power Spectrum and Implications for Hydrogen Epoch of Reionization Array

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    Unaccounted for systematics from foregrounds and instruments can severely limit the sensitivity of current experiments from detecting redshifted 21~cm signals from the Epoch of Reionization (EoR). Upcoming experiments are faced with a challenge to deliver more collecting area per antenna element without degrading the data with systematics. This paper and its companions show that dishes are viable for achieving this balance using the Hydrogen Epoch of Reionization Array (HERA) as an example. Here, we specifically identify spectral systematics associated with the antenna power pattern as a significant detriment to all EoR experiments which causes the already bright foreground power to leak well beyond ideal limits and contaminate the otherwise clean EoR signal modes. A primary source of this chromaticity is reflections in the antenna-feed assembly and between structures in neighboring antennas. Using precise foreground simulations taking wide-field effects into account, we provide a framework to set cosmologically-motivated design specifications on these reflections to prevent further EoR signal degradation. We show HERA will not be impeded by such spectral systematics and demonstrate that even in a conservative scenario that does not perform removal of foregrounds, HERA will detect EoR signal in line-of-sight kk-modes, k0.2hk_\parallel \gtrsim 0.2\,h~Mpc1^{-1}, with high significance. All baselines in a 19-element HERA layout are capable of detecting EoR over a substantial observing window on the sky.Comment: 11 pages, 6 figures (10 total including subfigures), submitted to Ap

    The dual pathway to information avoidance in information systems use

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    This article develops an explanatory model of information avoidance behavior from extant theory and examines its hypotheses using psychophysiological methods. It integrates existing but partially conflicting explanations into a coherent positivist model based on Coping Theory. The existence of two distinct but interlinked causal pathways to information avoidance will be outlined. Both pathways are cause by defects in the information quality. The first pathway is grounded on being threatened by the information’s inconsistency. The second pathway is based on being distressed by the information’s complexity. Due to the involvement of cognition as well as affect, the usefulness of traditional measurement methods alone is deemed to be limited. Thus, we will draw upon recent advances from NeuroIS research in order to integrate psychophysiological measures into an extended, triangulated measurement protocol. This article intends to contribute to this special issue in three ways. First, it shapes a theoretical model for studying information avoidance which has received little attention in IS research. Second, it exemplifies the derivation and instantiation of a NeuroIS measurement model and the selection of appropriate NeuroIS methods for scrutinizing the theoretical information avoidance model. Third, based on the evidence of an experiment, it provides guidelines for how to conduct eye-tracking, pupillometry, and facial electromyography measurements as well as how to subsequently derive meaning from the initial data collected

    The Indian-Atlantic Ocean gateway during the Pliocene: current dynamics and changing sediment provenance

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    The Pliocene epoch represents a discrete interval which reversed a long-term trend of late Neogene cooling and is also the most recent geological interval in which global temperatures were several degrees warmer than today. It is therefore often considered as the best analogue for a future anthropogenic greenhouse world. However, there is growing evidence that the Pliocene was not a stable period but can rather be subdivided in several distinct climate phases. Our understanding of Pliocene climate variability in the Southern Hemisphere, and especially in the Atlantic-Indian ocean gateway, is limited by scarce marine records and poor age control on existing terrestrial climate archives. At five from six drilling locations of IODP Exp. 361 (Jan. – March 2016) high resolution complete Plio-/Pleistocene sections have been recovered (see IODP Expedition 361 – Southern African Climates and Agulhas LGM Density Profile by Gruetzner et al., this Volume). Our new research proposal focuses on three of these sites forming a latitudinal transect in the Atlantic-/Indian Ocean gateway and combines chemical, physical property and seismic methods. Primary site for our investigations is Site U1475 with the focus on the interplay between northern and southern sourced deep water masses at the Agulhas Plateau. This will be augmented by investigations at Sites U1479 (Cape Basin) and U1474 (Natal Valley), both located in the pathway of modern NADW. Our research is driven by three main working hypotheses: Seismic stratigraphies for the last 6 Ma and sediment drift growth in the Atlantic-Indian gateway are mainly controlled by bottom water flow changes Using the new sediment archives and physical property records from IODP Exp. 361 (Hall et al., 2016) we aim to construct detailed seismic stratigraphies for the Agulhas Plateau, the Natal valley and the Cape basin for the last 6 Ma. At all Exp. 361 sites P-wave velocity and density records are of sufficient quality to enable detailed correlations of drilling results and site survey data through the calculation of synthetic seismograms. Our working hypothesis implies that seismic reflection patterns and sediment accumulation during the Pliocene are closely linked to deep water circulation changes associated with climate Pliocene phases. Furthermore four distinct high latitude Pliocene glaciation events have been identified. We speculate that these phases and events have led to deep water circulation changes in Agulhas region, have altered the sediment physical properties and thus may be recognized as reflectors in the seismic profiles. How did the sediment input of terrigenous vs. biogenic sediment components in the gateway change during these events? Are these changes driven by dilution, dissolution, or productivity? We strive to answer these questions by interpreting the physical and chemical (XRF) core scanning records. Trajectories and intensities of deep water masses in the Agulhas region during the Pliocene were influenced by Antarctic ice volume rather than by the closure of the Central American Seaway. The Exp. 361 drill sites offer the possibility to inter-correlate different flow speed proxies and to derive a detailed picture of flow changes during the Pliocene. By comparing core-measurements of sortable silt (S̅S̅), physical properties and XRF-core scanning data with seismic features we will tie the major flow speed changes to our seismic grid covering the Agulhas Plateau such that changing current intensities and pathways can be mapped together. Here we hypothesize that these changes are mainly driven by climate (Antarctic ice volume). What were the main changes associated with the Pliocene instability of Antarctic ice sheets and was the production of Antartic Bottom Water (AABW) reduced or enhanced during these intervals? How have the sedimentation patterns changed under the growing influence of North Atlantic Deep Water (NADW)? Was there also a potential influence of tectonic processes on the flow changes in the Agulhas region? Especially the closure of the Centarl American Seaway CAS between ~14 and ~2.7 Ma is thought to have had a profound impact on climate. The Pliocene variability in sediment provenance on millennial timescales is subdued when compared to the Pleistocene. Understanding the mechanisms and causes of abrupt climate change is one of the major challenges in global climate change research today and there is growing evidence that millennial scale climate variability was enhanced during times when a critical threshold in continental ice volume was surpassed. Dramatic millennial scale climate shifts are well documented for the “glacial world” of the late Pleistocene but are examined to a much lesser extent for earlier time periods. We suggest testing the potential threshold behaviour for the Atlantic-Indian gateway by comparing short term fluctuations in sediment composition and siliciclastic provenance in the Agulhas region before and after the onset of the Northern Hemisphere glaciation (NHG) at ~2.7 Ma. Time series of sediment provenance dated by “orbital tuning” will be analysed in the time and frequency domain to investigate at what times during the interval 2 – 6 Ma millennial scale climate variability was enhanced or subdued

    Untersuchung der Krustenstruktur des Manihiki Plateaus im Rahmen der Expedition SO-224

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    Das Manihiki Plateau ist ein untermeerisches Lavaplateau, eine sogenannte „Large Igneous Province“ (LIP), im zentralen Westpazifik (Abb. 1). Es ent-stand in der frühen Kreide (ca. 125 Ma) wahrscheinlich als ein Teilstück der „Super-LIP“ Ontong Java Nui (Chandler et al., 2013; 2012; Taylor, 2006). Dieses vulkanische Plateau bestand neben dem Manihiki Plateau aus dem Ontong Java Plateau und dem Hikurangi Plateau (Abb.1), sowie weiteren Teilstücken, die mittlerweile subduziert wurden (Larson et al., 2002; Viso et al., 2005). Man geht davon aus, dass Ontong Java Nui ungefähr 1% der Erd-oberfläche bedeckte. Eine vulkanische Provinz entsteht meist durch eine massive erste vulkanische Phase, gefolgt von mehreren kürzeren vulkani-schen Phasen (Coffin and Eldholm, 1994). Ontong Java Nui brach zwischen diesen zwei plateaubildenden Phasen auseinander (Hoernle et al., 2010; Timm et al., 2011), und die Teilplateaus durchliefen jeweils eine individuelle tektonische und petrologische Entwicklung. Während der Expedition SO-224 im Jahr 2012 wurden zwei refraktions- und weitwinkelreflexionsseismische Profile aufgenommen (Fig. 1). Hierzu wurden jeweils 33 Ozeanbodenseismometer ausgebracht. Diese Daten erlauben uns einen Einblick in die Struktur der Kruste und oberen Mantels des Manihiki Pla-teaus. Somit können die Hypothesen über die gemeinsame Entstehung des Manihiki Plateaus mit dem Ontong Java Plateau und dem Hikurangi Plateau überprüft werden. Ebenso ist es möglich, die Struktur der zwei größten Un-terprovinzen des Manihiki Plateaus, das High Plateau und die Western Plateaus, zu vergleichen. Bei der Modellierung der Krustenstruktur der beiden Unterprovinzen traten einige Gemeinsamkeiten, aber auch erstaunliche Unterschiede zu Tage (Abb. 2). Generell besteht eine LIP aus einer unteren Kruste, die sehr hohe P-Wellengeschwindigkeiten (7.1 bis 7.7 km/s) aufweist. Diese Schicht ist in bei-den Teilprovinzen vorhanden. Die Krustenmächtigkeit variiert zwischen 9 und 17 km an den Western Plateaus (Abb. 2a) und beträgt konstant 20 km am High Plateau (Abb. 2b). Die Struktur der oberen Kruste weist große Unter-schiede zwischen den verschiedenen Teilprovinzen auf. Das High Plateau ist durch basaltische Flussstrukturen geprägt. Zahlreiche intrusive und extrusive vulkanische Strukturen, wie beispielsweise Tiefseeberge sind hier belegt (Abb. 1 und 2b). Dies deutet auf eine massive vulkanische Aktivität während späte-rer vulkanischer Phasen hin. Im Gegensatz dazu zeigen die Western Pla-teaus nur einen sehr lokalen und geringen Vulkanismus. Mehrere Horst- und Grabensysteme sowie Sedimentbecken können dort identifiziert werden (Abb. 2a). Dieses deutet auf eine starke tektonische Deformation der Western Pla-teaus hin. Auch der graduelle Anstieg der Kruste-Mantelgrenze weist auf eine gedehnte Kruste hin (Abb. 2a). Somit zeigen die beiden Unterprovinzen des Manihiki Plateaus eine unterschiedliche Entwicklung nach ihrer gemeinsamen Entstehung als eines Teils von Ontong Java Nui. Das High Plateau wurde nur an seinen Rändern tektonisch beansprucht und durchlief weitere Phasen exzessiver vulkanischer Aktivität. Die Western Pla-teaus wurden wahrscheinlich starken Dehnungskräften im Zusammenhang mit dem Abbruch des Ontong Java Plateaus ausgesetzt. Somit liegt hier eine Dehnung der vorher entstandenen LIP-Kruste und geringer Vulkanismus vor. Diese Erkenntnisse können uns genaueren Aufschluss darüber geben, welche Prozesse den Aufbruch der „Super-LIP“ Ontong Java Nui begünstigt haben und stellen wichtige Rahmenbedingungen für eine plattentektonische Rekon-struktion des zentralen Westpazifiks in der Kreide dar. Durch eine Kartierung der Ränder und Beschaffenheit der Kruste der verschiedenen Teilplateaus Ontong Java Nuis können die ursprüngliche Positionierung der verschiedenen Plateaus zueinander rekonstruiert werden. Dies bildet die Grundlage einer er-folgreichen plattenkinematischen Rekonstruktion

    A new seismic stratigraphy for the Agulhas Plateau resembles major paleo-oceanographic changes in the Indian-Atlantic Ocean gateway since the late Miocene

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    The exchange of shallow and deep water masses between the Indian Ocean and the Atlantic constitutes an integral inter-ocean link in the global thermohaline circulation. In the gateway south of South Africa long-term changes in deep water flow during the Cenozoic have been initially studied using seismic reflection profiles. But the seismic stratigraphy was poorly constrained and not further resolved within the time period from the late Miocene to present. In particular, there were limited Pliocene records that could be used to investigate the influence of climatic (e.g. Antarctic ice volume) and tectonic (e.g. closure of the Central American seaway) on the deep-water variability. In 2016 the International Ocean Discovery Program (IODP) Expedition 361 (“SAFARI”) recovered complete high-resolution Plio-/Pleistocene sediment sections at six drilling locations on the southeast African margin and in the Indian-Atlantic ocean gateway. Here, we present results from Site U1475 (Agulhas Plateau), a location proximal to the entrance of North Atlantic Deep Water (NADW) to the Southern Ocean and South Indian Ocean. The site is located over a sediment drift in 2669 m water depth and comprises a complete carbonate rich (74 – 85%) stratigraphic section of the last ~7 Ma. We edited high-resolution data sets of density, velocity and natural gamma radiation measured at Site U1475 and corrected them to in-situ conditions. Cross correlations show that acoustic impedance contrasts and thus the formation of seismic reflectors are mainly due to density changes that are caused by climate-induced variations in biogenic vs. terrigenous sediment input. The calculated synthetic seismograms show an excellent correlation of drilling results with the site survey seismic field record, provide an accurate traveltime to depth conversion, and allow preliminary age assignments (± 0.3 Ma) based on the shipboard bio- and magnetostratigraphy. The most prominent reflectors are associated with compositional changes related to late Pleistocene glacial/interglacial variability, the middle Pleistocene transition, and the onset of the northern hemisphere glaciation. Furthermore, a peculiar early Pliocene interval (~ 5.3 – 4.0 Ma) bounded by two reflectors is characterized by 3-fold elevated sedimentation rates (> 10 cm/ka) and the occurrence of sediment waves. We argue that this enhanced sediment transport to the Agulhas Plateau was caused by a reorganization of the bottom current circulation pattern due to maximized inflow of NADW. Rhythmic bedding within the Pliocene sediment wave sequence likely reflects the 100-kyr orbital cycle. On the other hand, colour reflectance and natural gamma radiation show highest variability in the precession band. The very regular response of the core logging data to orbital forcing suggests that the shipboard age model can be significantly improved by cyclostratigraphy
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