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  • 2010-2014  (30)
  • 1995-1999
  • 2011  (30)
  • 1
    Keywords: Forschungsbericht
    Type of Medium: Online Resource
    Pages: Online-Ressource (47 S., 19,63 MB) , Ill., graph. Darst., Kt.
    Series Statement: IFM-GEOMAR report 42
    Language: English
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  • 2
    Keywords: Hochschulschrift ; Mittelamerika ; Kontinentalabhang ; Subduktion
    Type of Medium: Online Resource
    Pages: Online-Ressource (PDF-Datei: XVI, 111 S., 27,7 MB)
    Language: English
    Note: Auch als gedrucktes Dok. erschienen , Kiel, Univ., Diss., 2011
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  • 3
  • 4
    Publication Date: 2018-03-13
    Description: Active ridge propagation frequently occurs along spreading ridges and profoundly affects ridge crest segmentation over time. The mechanisms controlling ridge propagation, however, are poorly understood. At the slow spreading Mid-Atlantic Ridge at 21.5°N a seismic refraction and wide-angle reflection profile surveyed the crustal structure along a segment controlled by rapid ridge propagation. Tomographic traveltime inversion of seismic data suggests that the crustal structure along the ridge axis is controlled by melt supply; thus, crust is thickest, 8 km, at the domed segment center and decreases in thickness toward both segment ends. However, thicker crust is formed in the direction of ridge propagation, suggesting that melt is preferentially transferred toward the propagating ridge tip. Further, while seismic layer 2 remains constant along axis, seismic layer 3 shows profound changes in thickness, governing variations in total crustal thickness. This feature supports mantle upwelling at the segment center. Thus, fluid basaltic melt is redistributed easily laterally, while more viscose gabbroic melt tends to crystallize and accrete nearer to the locus of melt supply. The onset of propagation seems to have coincided with the formation of thicker crust, suggesting that propagation initiation might be due to changes in the melt supply. After a rapid initiation a continuous process of propagation was established. The propagation rate seems to be controlled by the amount of magma that reaches the segment ends. The strength of upwelling may govern the evolution of ridge segments and hence ultimately controls the propagation length.
    Type: Article , PeerReviewed
    Format: text
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  • 5
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    AGU (American Geophysical Union)
    In:  Journal of Geophysical Research: Solid Earth, 116 (B10). B10305.
    Publication Date: 2019-09-23
    Description: We developed thermal models for the Chile subduction zone along two profiles at 38.2°S and 42°S within the rupture area of the 1960 M = 9.5 Valdivia earthquake and south of the 2010 M = 8.8 Maule earthquake. The age difference of the subducting Nazca Plate has a major impact on the thermal regime, being much younger and hotter in the south. Seafloor heat flow observations confirm this difference but also indicate that in the southern area, heat advection at the outer rise cools the incoming plate. Heat flow values derived from the depth of gas hydrate bottom-simulating reflectors are in general agreement with probe and borehole measurements. The positions where the plate interface reaches temperatures of 100–150°C and 350–450°C differ between the two profiles. If these temperatures control the updip and downdip limits of the interplate seismogenic zone, the seismogenic zone widens and shifts landward to greater depths from south to north. Observed microseismicity, however, seems to fade at temperatures much lower than 350–450°C. This discrepancy can be explained in three alternative ways: (1) deformation in a thick subduction channel controls the seismic/aseismic transition; (2) microseismicity recorded over a limited time period does not represent the rupture depth of large interface earthquakes; or (3) the serpentinized mantle wedge controls the downdip limit.
    Type: Article , PeerReviewed
    Format: text
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  • 6
    Publication Date: 2013-02-28
    Description: EGU2011-12780 A temporary passive seismic network of 31 broad-band stations was deployed in the region around Talca and Constitución between 35°S to 36°S latitude and 71°W to 72.5°W longitude. The network was operated between March and October 2008. Thus, we recorded data prior the magnitude Mw=8.8 earthquake of 27 February 2010 at a latitude of the major slip and surface uplift. The experiment was conducted to address fundamental questions on deformation processes, crustal and mantle structures, and fluid flow. We present results of a teleseismic P receiver function study that covers the coastal region and reaches to the Andes. The aim is to determine the structure and thickness of the continental crust and constrain the state of hydration of the mantle wedge. The P-wave receiver function technique requires large teleseismic earthquakes from different distances and backazimuths. A few percent of the incident P-wave energy from a teleseismic event will be converted into S-wave (Ps) at significant and relatively sharp discontinuities beneath the station. A small converted S phase is produced that arrives at the station within the P wave coda directly after the direct P-wave. The converted Ps phase and their crustal multiples contain information about crustal properties, such as Moho depth and the crustal vp/vs ratio. We use teleseismic events with magnitudes mb 〉 5.5 at epicentral distances between 30° and 95° to examine P-to-S converted seismic phases. Our preliminary results provide new information about the thickness of the continental crust beneath the coastal region in Central Chile. At most of the stations we observed significant energy from P to S converted waves between 4 and 5 s after the direct P-wave within a positive phase interpreted as the Moho, occurring at 35 to 40 km. The great Maule earthquake of 27 February 2010 nucleated up-dip of the continental Moho. The rupture of this earthquake seems to have propagated down-dip of the Moho. The Moho reflection show a positive polarity, indicating that the mantle is either dry or only moderately hydrated. We observed converted energy from an intracrustal boundary at around 2 s that disappears near the coast. Further, positive polarity peaks occur that are possibly caused by the down going plate.
    Type: Conference or Workshop Item , NonPeerReviewed
    Format: text
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  • 7
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    In:  [Poster] In: 71. Jahrestagung der Deutschen Geophysikalischen Gesellschaft, 21.-24.02.2011, Köln .
    Publication Date: 2012-02-23
    Description: The Tyrrhenian Basin is the youngest basin of the Western Mediterranean Sea. It is assumed that the rifting and opening of the basin is caused by slab rollback during the latest phases of subduction of several segments of the Tethys oceanic lithosphere. Rifting processes in the Tyrrhenian have been continuous since the late Miocene. The advantages of studying this young basin are the well preserved, undeformed conjugated margins which are close to each other and covered only by thin sediments. Furthermore, the extension factor increases from North to South making it possible to investigate different stages of rift structures. This makes the Tyrrhenian Basin a unique natural laboratory to study continental break-up and rift processes which are still not fully understood. In a collaborative project with partners from Spain and Italy new seismic data were acquired during a two-ship experiment in April and May 2010. The Spanish vessel Sarmiento de Gamboa operated an airgun array and a 4 km long seismic streamer for collecting MCS data. The Italian vessel Urania was used for deployment and recovery of 25 IFM-GEOMAR Ocean-Bottom-Hydrophones which were recording refraction and wide-angle seismic data on that profiles. At the DGG 2011 we will present first results of a seismic transect crossing the Tyrrhenian Sea between Sardinia and Italy at 41°N.
    Type: Conference or Workshop Item , NonPeerReviewed
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  • 8
    Publication Date: 2012-02-23
    Type: Conference or Workshop Item , NonPeerReviewed
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  • 9
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    In:  [Talk] In: Gemeinsames Kolloquium der Schwerpunktprogramme ICDP - International Continental Scientific Drilling Program und IODP - Integrated Ocean Drilling Program, 14.03.-16.03.2011, Münster .
    Publication Date: 2012-07-06
    Description: Interplate earthquakes in subduction zones are generated in the seismogenic zone, i.e. the segment of the plate boundary where unstable slip occurs. Understanding the mechanisms that control the updip and downdip limits of this zone, as well as the nature and role of asperities within it, provide significant insights into the rupture size and dynamics of the world’s largest earthquakes. The Costa Rica Seismogenesis Project (CRISP) is designed to understand the processes that control nucleation and seismic rupture propagation of large earthquakes at erosive subduction zones (Ranero et al. 2007). In 2002 a magnitude Mw=6.4 earthquake may have nucleated at the subduction thrust to be penetrated and sampled by CRISP, 40 km west of Osa Peninsula (Figure 1). However, global event localization is associated with too large errors to prove that the event actually occurred at a location and depth to be reachable by riser drilling. We have compiled a database including foreshocks, the main shock, and ~400 aftershocks, with readings from all the seismological networks that recorded the 2002 Osa sequence locally (Figure 1). This includes a temporal network of oceanbottom hydrophones (OBH) that happened to be installed close to the area (Arroyo et al. 2009). The greatly improved coverage provided by the OBH enable us to better constrain the event relocations that we are presently undertaking. Within the frame of a proposal recently submitted to DFG with IODP emphasis, detailed inspection of the data and 3-D data modelling will be carried out to yield source parameters that can be rated against structural information from seismic and drilling constraints. Moreover, teleseismic waveform inversion will provide additional constraints for the centroid depth of the 2002 Osa earthquake, allowing further study of the focal mechanism. This sequence is the latest at the Costa Rican seismogenic zone to date, in a segment of the erosional margin where seamount-covered oceanic floor is presently subducting (Figure 1). It took place trenchward from a 1999 Mw=6.9 earthquake sequence, that it is thought to have been nucleated by a seamount acting like an asperity (Bilek et al. 2003). The work proposed here aims to provide definite evidence that the planned Phase B of CRISP will be successful in drilling the seismogenic coupling zone. Furthermore, the seismological data will be interpreted jointly with thermal and drilling data from IODP Expedition 334 to refine the link between temperature and seismogenesis at erosive convergent margins.
    Type: Conference or Workshop Item , NonPeerReviewed
    Format: text
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  • 10
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    Forschungszentrum Jülich, Projektträger Biologie, Energie, Ökologie, Bereich Meeres- und Polarforschung
    In:  [Talk] In: Statusseminar Meeresforschung mit FS Sonne 2011, 09.-10.02.2011, Hannover . Tagungsband / Meeresforschung mit FS Sonne : Statusseminar 2011 ; pp. 141-144 .
    Publication Date: 2012-07-06
    Type: Conference or Workshop Item , NonPeerReviewed
    Format: text
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