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  • 1
    Keywords: Hochschulschrift ; Maule-Gebiet ; Subduktion ; Seismik
    Type of Medium: Online Resource
    Pages: 1 Online-Ressource ( 147Seiten = 42MB) , graph. Darst.
    DDC: 551.8098335
    Language: English
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  • 2
    Keywords: Hochschulschrift ; Subduktion ; Seismik ; Maule-Gebiet
    Type of Medium: Online Resource
    Pages: Online-Ressource
    DDC: 551.8098335
    Language: English
    Note: Kiel, Univ., Diss., 2011
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  • 3
    Keywords: Hochschulschrift ; Maule-Gebiet ; Subduktion ; Seismik
    Type of Medium: Book
    Pages: XXIV, 121 S. , graph. Darst.
    DDC: 551.8098335
    Language: English
    Note: Kiel, Univ., Diss., 2011
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  • 4
    Publication Date: 2020-02-06
    Description: Highlights • 2-D velocity models at the highest slip patch during the Chilean 2010 Mw 8.8 earthquake. • The highest slip patch correlates with large accretionary prisms. • The highest slip patch correlates with low continental slope angles. • A similar pattern is observed along the giant 1960 Mw 9.5 earthquake rupture area. Abstract Subduction megathrust earthquakes show complex rupture behaviour and large lateral variations of slip. However, the factors controlling seismic slip are still under debate. Here, we present 2-D velocity-depth tomographic models across four trench-perpendicular wide angle seismic profiles complemented with high resolution bathymetric data in the area of maximum coseismic slip of the 8.8 Maule 2010 megathrust earthquake (central Chile, 34°–36°S). Results show an abrupt lateral velocity gradient in the trench-perpendicular direction (from 5.0 to 6.0 km/s) interpreted as the contact between the accretionary prism and continental framework rock whose superficial expression spatially correlates with the slope-shelf break. The accretionary prism is composed of two bodies: (1) an outer accretionary wedge (5–10 km wide) characterized by low seismic velocities of 1.8–3.0 km/s interpreted as an outer frontal prism of poorly compacted and hydrated sediment, and (2) the middle wedge (∼50 km wide) with velocities of 3.0–5.0 km/s interpreted as a middle prism composed by compacted and lithified sediment. In addition, the maximum average coseismic slip of the 2010 megathrust event is fairly coincident with the region where the accretionary prism and continental slope are widest (50–60 km wide), and the continental slope angle is low (〈5°). We observe a similar relation along the rupture area of the largest instrumentally recorded Valdivia 1960 9.5 megathrust earthquake. For the case of the Maule event, published differential multibeam bathymetric data confirms that coseismic slip must have propagated up to ∼6 km landwards of the deformation front and hence practically the entire base of the middle prism. Sediment dewatering and compaction processes might explain the competent rheology of the middle prism allowing shallow earthquake rupture. In contrast, the outer frontal prism made of poorly consolidated sediment has impeded the rupture up to the deformation front as high resolution seismic reflection and multibeam bathymetric data have not showed evidence for new deformation in the trench region.
    Type: Article , PeerReviewed
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  • 5
    Publication Date: 2019-09-23
    Description: Reloca Slide is the relict of an ~24 km³ submarine slope collapse at the base of the convergent continental margin of central Chile. Bathymetric and seismic data show that directly to the north and south of the slide the lower continental slope is steep (~10°), the deformation front is shifted landwards by 10–15 km, and the frontal accretionary prism is uplifted. In contrast, ~80 km to the north the lower continental margin presents a lower slope angle of about 4° and a wide frontal accretionary prism. We propose that high effective basal friction conditions at the base of the accretionary prism favored basal accretion of sediment and over-steepening of the continental slope, producing massive submarine mass wasting in the Reloca region. This area also spatially correlates with a zone of low coseismic slip of the 2010 Maule megathrust earthquake, which is consistent with high basal frictional coefficients.
    Type: Article , PeerReviewed
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  • 6
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    In:  [Talk] In: The Lübeck Retreat, Collaborative Research Centre SFB 574 Volatiles and Fluids in Subduction Zones: Climate Feedback and Trigger Mechanisms for Natural Disasters, 23.05.-25.05.2012, Lübeck . The Lübeck Retreat, Collaborative Research Centre SFB 574 Volatiles and Fluids in Subduction Zones: Climate Feedback and Trigger Mechanisms for Natural Disasters : final colloquium of SFB 574 ; May 23-25, 2012; program & abstracts ; p. 1 .
    Publication Date: 2019-09-23
    Description: Within the project SFB574, an “amphibious” network of 15 ocean bottom seismometers and 27 land stations was operated from April to October 2008 along 350 km from the outer-rise to the magmatic arc. Additional readings from 11 permanent stations of the Chilean Seismological Service were included in the database improving onshore coverage. One of the main goals of the project is to gain a detailed image of the crustal and upper mantle structure and the seismogenic zone by analyzing earthquake distribution and combined passive and active source seismic tomographic images. To achieve precise earthquake locations and to serve as an initial model for local earthquake tomography, we derived a P- and S-wave minimum-1D model using a very high-quality subset of 340 events (GAP ! 180°, at least 10 P-wave and 5 S-wave arrivals) and velocity information from a wideangle profile shot in the area. Most of the ~1200 earthquakes recorded in our target area were originated within the subducting slab down to ~140 km depth, with a higher concentration beneath the main cordillera, at depths of 80-110 km. Fewer events were generated at the outer-rise, at depths of ~20-40 km, closely following the NE-SW trend of the oceanic plate faulting. The database was relocated using the minimum 1-D model and a subset of 400 events (GAP ! 180°, at least 8 P-wave arrivals) with ~7000 observations was selected to perform a P-wave tomography. Our results confirm the strong, lateral velocity gradient in the forearc seen in previous works along the margin, interpreted as the transition between a paleoaccretionary complex and the seaward edge of the Paleozoic continental framework. The downdip limit of the interplate seismicity previous to the great earthquake was aparently controlled by a low-velocity anomaly at ~40 km depth, shallower than the deeper extent estimated by geodetic modeling of the rutpture and from aftershocks relocation for the Maule earthquake. The interplate seismicity nucleated from ~40 up to ~20 km depth, and did not extend up to the 100°C isotherm. It was sparse except for a cluster of ~1200 km2 offshore and SW of Pichilemu town, within an area where a locking " 75 % before the great earthquake has been estimated. The deep outer-rise seismicity and the low velocities on top suggest considerable hydration of the downgoing plate.
    Type: Conference or Workshop Item , NonPeerReviewed
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  • 7
    Publication Date: 2019-09-23
    Description: The 27 February, 2010 Maule earthquake (Mw=8.8) ruptured ~600 km of the Nazca-South America plate boundary (33°S-38.5°S) and caused hundreds of fatalities and billions of dollars in structural losses. In order to better understand the coseismic rupture process of this devastating earthquake, we study the seismic velocity structure of the Nazca-South America subduction zone near the epicentral region. The results show a wedge shaped body ~40 km wide with typical sedimentary velocities (〈3.5 km/s) interpreted as an active accretionary prism composed of weak and fluid-rich sediments. Landward of the imaged accretionary prism, the velocity model shows an abrupt velocity-contrast suggesting a rheological and lithological change which is interpreted as a backstop. The backstop is coincident with the seaward limit of the aftershocks, defining the seismic front and up-dip limit of the megathrust earthquake. The latter is also observed along strike (33°S-38.5°S) where the seaward extension of more than 1000 aftershocks is located at roughly the same distance from the deformation front (~30 km). On the other hand, reflections from the top of the subducting oceanic crust constraint the location of the plate boundary and its dip angle to 10° and thus we estimate the hypocenter location at 22±1 km depth. Our seismic results provide crucial constraints for evaluating the capability of this area to target shallow tsunamigenic earthquakes and assessing earthquake and tsunami hazard.
    Type: Conference or Workshop Item , NonPeerReviewed
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  • 8
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    In:  (PhD/ Doctoral thesis), Christian-Albrechts-Universität, Kiel, 119 pp
    Publication Date: 2012-07-06
    Description: During the last decades, the Chilean margin offshore Maule (34±S −36±S) had been reported as a highly locked and seismically quiet zone. The stress-accumulated state finished on the 27th of February 2010, when a megathrust earthquake (with Mw = 8.8) ruptured » 400 km of the Nazca-South America plate boundary. Unfortunately, up to now little was known about the seismic structure offshore Maule. In the frame of the third phase of the project SFB 574 “Volatiles and Fluids in Subduction Zones” of the Christan-Albrechts University of Kiel, seismic data was analyzed in order to obtain detailed images of the deep structure of the margin and of the outer rise. Here are presented constraints on the forearc and the subduction zone structure of the rupture area derived from seismic refraction and wide-angle data. The results show a wedge shaped body » 40 km wide with typical sedimentary velocities interpreted as a frontal accretionary prism (FAP). Landward of the imaged FAP, the velocity model shows an abrupt velocity-contrast suggesting a lithological change, which is interpreted as the contact between the FAP and the paleo accretionary prism (backstop). The backstop location is coincident with the seaward limit of the aftershocks, defining the updip limit of the co-seismic rupture and the seismogenic zone. Furthermore, the seaward limit of the aftershocks coincides with the location of the shelf break in the entire earthquake rupture area (33.5±S−38.5±S), which is interpreted as the location of the backstop along the margin. Published seismic profiles at the northern and southern limit of the rupture area also show the presence of a strong horizontal velocity gradient imaging the seismic backstop at a distance of » 30 km from the deformation front. The seismic wide-angle reflections from the top of the subducting oceanic crust constrain the location of the plate boundary offshore, dipping » 10±. The projection of the epicenter of the Maule earthquake onto our derived interplate boundary yielded a hypocenter around 20 km depth. This implies that the earthquake nucleated somewhere within the seismogenic zone, neither at its updip nor at its downdip limit. The second part of this thesis focuses on the dependency between the incoming plate’s bend faulting, lithospheric hydration and shallow outer rise seismic activity. To support the interpretation, are presented Vp and Vs seismic models obtained from wide angle seismic data and the derived 2D Poisson’s ratio distribution at the outer rise. The oceanic lithosphere shows a high degree of hydration, due to the water infiltration through the bending-related faults exposed to seawater. This process is presumably intensified bythe existence of a seamount in the area. It is concluded that the water infiltrates deep into the lithosphere, triggering shallow earthquakes in the outer rise and likely serpentinization in the mantle, estimated to be about 10%.
    Type: Thesis , NonPeerReviewed
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  • 9
    Publication Date: 2017-06-08
    Description: The 27 February, 2010 Maule earthquake (Mw=8.8) ruptured ~400 km of the Nazca-South America plate boundary and caused hundreds of fatalities and billions of dollars in material losses. Here we present constraints on the fore-arc structure and subduction zone of the rupture area derived from seismic refraction and wide-angle data. The results show a wedge shaped body ~40 km wide with typical sedimentary velocities interpreted as a frontal accretionary prism (FAP). Landward of the imaged FAP, the velocity model shows an abrupt velocity-contrast, suggesting a lithological change which is interpreted as the contact between the FAP and the paleo accretionary prism (backstop). The backstop location is coincident with the seaward limit of the aftershocks, defining the updip limit of the co-seismic rupture and seismogenic zone. Furthermore, the seaward limit of the aftershocks coincides with the location of the shelf break in the entire earthquake rupture area (33°S–38.5°S), which is interpreted as the location of the backstop along the margin. Published seismic profiles at the northern and southern limit of the rupture area also show the presence of a strong horizontal velocity gradient seismic backstop at a distance of ~30 km from the deformation front. The seismic wide-angle reflections from the top of the subducting oceanic crust constrain the location of the plate boundary offshore, dipping at ~10°. The projection of the epicenter of the Maule earthquake onto our derived interplate boundary yielded a hypocenter around 20 km depth, this implies that this earthquake nucleated somewhere in the middle of the seismogenic zone, neither at its updip nor at its downdip limit.
    Type: Article , PeerReviewed
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  • 10
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    Servicio Nacional de Geología y Minería (SERNAGEOMIN)
    In:  Andean Geology, 39 (3). pp. 564-572.
    Publication Date: 2016-09-05
    Description: Most of the recent published geodetic models of the 2010 Maule, Chile mega-thrust earthquake (Mw=8.8) show a pronounced slip maximum of 15-20 m offshore Iloca (similar to 35 degrees S), indicating that co-seismic slip was largest north of the epicenter of the earthquake rupture area. A secondary slip maximum 8-10 m appears south of the epicenter west of the Arauco Peninsula. During the first weeks following the main shock and seaward of the main slip maximum, an outer rise seismic cluster of 〉450 events, mainly extensional, with magnitudes Mw=4-6 was formed. In contrast, the outer rise located seaward of the secondary slip maximum presents little seismicity. This observation suggests that outer rise seismicity following the Maule earthquake is strongly correlated with the heterogeneous coseismic slip distribution of the main megathrust event. In particular, the formation of the outer-rise seismic cluster in the north, which spatially correlates with the main maximum slip, is likely linked to strong extensional stresses transfered from the large slip of the subducting oceanic plate. In addition, high resolution bathymetric data reveals that bending-related faulting is more intense seaward of the main maximum slip, where well developed extensional faults strike parallel to the trench axis. Also published seismic constraints reveal reduced P-wave velocities in the uppermost mantle at the trench-outer rise region (7.5-7.8 km/s), which suggest serpentinization of the uppermost mantle. Seawater percolation up to mantle depths is likely driven by bending related-faulting at the outer rise. Water percolation into the upper mantle is expected to be more efficient during the co-seismic and early post-seismic periods of large megathrust earthquakes when intense extensional faulting of the oceanic lithosphere
    Type: Article , PeerReviewed
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