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  • 1
    Publication Date: 2021-02-08
    Description: The AlpArray programme is a multinational, European consortium to advance our understanding of orogenesis and its relationship to mantle dynamics, plate reorganizations, surface processes and seismic hazard in the Alps–Apennines–Carpathians–Dinarides orogenic system. The AlpArray Seismic Network has been deployed with contributions from 36 institutions from 11 countries to map physical properties of the lithosphere and asthenosphere in 3D and thus to obtain new, high-resolution geophysical images of structures from the surface down to the base of the mantle transition zone. With over 600 broadband stations operated for 2 years, this seismic experiment is one of the largest simultaneously operated seismological networks in the academic domain, employing hexagonal coverage with station spacing at less than 52 km. This dense and regularly spaced experiment is made possible by the coordinated coeval deployment of temporary stations from numerous national pools, including ocean-bottom seismometers, which were funded by different national agencies. They combine with permanent networks, which also required the cooperation of many different operators. Together these stations ultimately fill coverage gaps. Following a short overview of previous large-scale seismological experiments in the Alpine region, we here present the goals, construction, deployment, characteristics and data management of the AlpArray Seismic Network, which will provide data that is expected to be unprecedented in quality to image the complex Alpine mountains at depth.
    Type: Article , PeerReviewed
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  • 2
    Publication Date: 2020-02-06
    Description: Proxy-based indicators of past climate change show that current global climate models systematically underestimate Holocene-epoch climate variability on centennial to multi-millennial timescales, with the mismatch increasing for longer periods1,2,3,4,5. Proposed explanations for the discrepancy include ocean–atmosphere coupling that is too weak in models6, insufficient energy cascades from smaller to larger spatial and temporal scales7, or that global climate models do not consider slow climate feedbacks related to the carbon cycle or interactions between ice sheets and climate4. Such interactions, however, are known to have strongly affected centennial- to orbital-scale climate variability during past glaciations8,9,10,11, and are likely to be important in future climate change12,13,14. Here we show that fluctuations in Antarctic Ice Sheet discharge caused by relatively small changes in subsurface ocean temperature can amplify multi-centennial climate variability regionally and globally, suggesting that a dynamic Antarctic Ice Sheet may have driven climate fluctuations during the Holocene. We analysed high-temporal-resolution records of iceberg-rafted debris derived from the Antarctic Ice Sheet, and performed both high-spatial-resolution ice-sheet modelling of the Antarctic Ice Sheet and multi-millennial global climate model simulations. Ice-sheet responses to decadal-scale ocean forcing appear to be less important, possibly indicating that the future response of the Antarctic Ice Sheet will be governed more by long-term anthropogenic warming combined with multi-centennial natural variability than by annual or decadal climate oscillations.
    Type: Article , PeerReviewed
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  • 3
    Publication Date: 2017-05-17
    Description: The causes for the formation of large igneous provinces and hotspot trails are still a matter of considerable dispute. Seismic tomography and other studies suggest that hot mantle material rising from the core-mantle boundary (CMB) might play a significant role in the formation of such hotspot trails. An important area to verify this concept is the South Atlantic region, with hotspot trails that spatially coincide with one of the largest low-velocity regions at the CMB, the African large low shear-wave velocity province. The Walvis Ridge started to form during the separation of the South American and African continents at ca. 130 Ma as a consequence of Gondwana breakup. Here, we present the first deep-seismic sounding images of the crustal structure from the landfall area of the Walvis Ridge at the Namibian coast to constrain processes of plume-lithosphere interaction and the formation of continental flood basalts (Paraná and Etendeka continental flood basalts) and associated intrusive rocks. Our study identified a narrow region (〈100 km) of high-seismic-velocity anomalies in the middle and lower crust, which we interpret as a massive mafic intrusion into the northern Namibian continental crust. Seismic crustal reflection imaging shows a flat Moho as well as reflectors connecting the high-velocity body with shallow crustal structures that we speculate to mark potential feeder channels of the Etendeka continental flood basalt. We suggest that the observed massive but localized mafic intrusion into the lower crust results from similar-sized variations in the lithosphere (i.e., lithosphere thickness or preexisting structures)
    Type: Article , PeerReviewed
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  • 4
    Publication Date: 2020-02-06
    Description: Highlights • Up to 33 km thick dominantly gabbroic crust beneath Walvis Ridge • Massive gabbro addition with subjacent cumulates to the COB south of Walvis Ridge. • Slow upper mantle at ~ 35 km depth beneath Etendeka Plateau • 4–6 km thick oceanic crust in the Angola Basin north of Florianopolis Transform • Velocity models suggest a dominant tectonic control on the location of magmatism. Abstract Voluminous magmatism during the South Atlantic opening has been considered as a classical example for plume related continental breakup. We present a study of the crustal structure around Walvis Ridge, near the intersection with the African margin. Two wide-angle seismic profiles were acquired. One is oriented NNW–SSE, following the continent–ocean transition and crossing Walvis Ridge. A second amphibious profile runs NW–SE from the Angola Basin into continental Namibia. At the continent–ocean boundary (COB) the mafic crust beneath Walvis Ridge is up to 33 km thick, with a pronounced high-velocity lower crustal body. Towards the south there is a smooth transition to 20–25 km thick crust underlying the COB in the Walvis Basin, with a similar velocity structure, indicating a gabbroic lower crust with associated cumulates at the base. The northern boundary of Walvis Ridge towards the Angola Basin shows a sudden change to oceanic crust only 4–6 km thick, coincident with the projection of the Florianopolis Fracture Zone, one of the most prominent tectonic features of the South Atlantic ocean basin. In the amphibious profile the COB is defined by a sharp transition from oceanic to rifted continental crust, with a magmatic overprint landward of the intersection of Walvis Ridge with the Namibian margin. The continental crust beneath the Congo Craton is 40 km thick, shoaling to 35 km further SE. The velocity models show that massive high-velocity gabbroic intrusives are restricted to a narrow zone directly underneath Walvis Ridge and the COB in the south. This distribution of rift-related magmatism is not easily reconciled with models of continental breakup following the establishment of a large, axially symmetric plume in the Earth's mantle. Rift-related lithospheric stretching and associated transform faulting play an overriding role in locating magmatism, dividing the margin in a magma-dominated southern and an essentially amagmatic northern segment.
    Type: Article , PeerReviewed
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  • 5
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    In:  [Talk] In: EGU General Assembly 2013, 07.-12.04.2013, Vienna, Austria .
    Publication Date: 2013-04-09
    Type: Conference or Workshop Item , NonPeerReviewed
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  • 6
    Publication Date: 2012-07-06
    Description: Earth processes related to incipient continent-continent collision have been studied via the example of Cyprus and the Eratosthenes Seamount in the eastern Mediterranean. Subduction of the African plate beneath the Cyprus-Anatolian plate continued until the seamount, and perhaps a predecessor, the Hecataeus Rise, approached the Cyprus arc trench. The following transition from subduction to collision triggered a series of synchronous deformations across the collision zone between Africa-Sinai-Arabia and Eurasia-Anatolia, including the entire eastern Mediterranean region. This fundamental Earth process has been studied during research cruise MSM14/3 with RV Maria S. Merian in spring 2010. 39 MCS-profiles of more than 2300 km entire length, more than 3000 km magnetic and sediment echosounder data, and about 4000 km of gravity data have been recorded. Four wide-angle reflection/refraction profiles across the seamount were measured with up to 34 OBS deployments along each profile. 10 ocean-bottommagnetotelluric stations were deployed along one of these profiles that connects the seamount with the Hecataeus Rise. One 650 km long amphibian refraction profile strikes across the seamount, Cyprus and southern Turkey. Of the 250 land stations, 200 were deployed in southern Turkey and 50 in Cyprus. A first analysis of the collected data led to the following hypothesis about the interrelation of observed processes: Continent-continent collision caused a compressional regime in the crustal lithosphere, which resulted in the flexure (of the Eratosthenes Seamount), uplift (of Cyprus and Turkey) and accordingly an increased tilt of the facing slopes. The collision reactivated Mesozoic fault lineaments in the Levantine Basin like the Baltim-Hecataeus-Line and created the Hecataeus Rise. Shortening in the non-consolidated Messinian to Holocene sediment succession between the seamount and Cyprus resulted in faulting, folding and compressional salt diapirism. The increase in pore pressure causes fluid migration and mud volcanism. Slope tilt and faulting triggered mass wasting. All of these processes are still shaping the seafloor morphology and interact with the bottom current circulation, which is reflected by sediment drift deposition, sediment remobilisation and erosion, which facilitates again mass wasting.
    Type: Conference or Workshop Item , NonPeerReviewed
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  • 7
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    In:  (Diploma thesis), Christian-Albrechts-Universität, Kiel, Kiel, Germany, 92 pp
    Publication Date: 2020-01-27
    Type: Thesis , NonPeerReviewed
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  • 8
    Publication Date: 2012-12-18
    Type: Conference or Workshop Item , NonPeerReviewed
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  • 9
    Publication Date: 2019-09-23
    Description: Several aspects of the formation and rifting of crust in backarc environments, like the Lau Basin in the SW Pacific, are still under question. A major unresolved question is, at what stage in the structural and thermal evolution of arc rifting does magmatism begin? The Fonualei Rift and Spreading Centre in Northeastern Lau Basin separates the Tonga Volcanic Arc from the Lau Backarc Basin and shows a strong gradient in the opening rate from South to North. The rift represents an ideal study site to investigate the formation and rifting of backarc crust at different stages of its tectonic and magmatic evolution. During the multidisciplinary cruise SO267 of RV Sonne (project ARCHIMEDES I), which sailed from Dec. 11, 2018 to Jan. 26, 2019, coincident seismic refraction and reflection profiles were acquired to image the deep crustal structure covering different sections of the Fonualei Rift and Spreading Centre. A total of 50 OBS from the GEOMAR pool were available for the refraction lines. Instruments were spaced at an average distance of 6 km and recorded arrivals from up 120 km offset. Seismic phases show little to no sediment cover on the seabed. Clear mantle arrivals (PmP and Pn) were recorded by the majority of stations and will allow the assessment of crustal thickness and upper mantle velocities. Additional geophysical data included gravity, magnetics and high-resolution bathymetry as well as Parasound and heatflow data, which were acquired along all profiles and will contribute to the tectonic interpretation of this complex region that is characterized by a number of microplates, active and abandoned spreading centres and transfer zones. This contribution will present an overview of the major scientific questions driving the ARCHIMEDES I project and present first results from the acquired seismic profiles, which aim to reveal the crustal architecture and the opening history of the Lau Basin.
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  • 10
    Publication Date: 2013-04-09
    Type: Conference or Workshop Item , NonPeerReviewed
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