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  • 2005-2009  (19)
  • 1990-1994
  • 2009  (19)
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  • 2005-2009  (19)
  • 1990-1994
Year
  • 1
    In: Marine and petroleum geology, Amsterdam [u.a.] : Elsevier Science, 1984, 26(2009), 6, Seite 795-804, 0264-8172
    In: volume:26
    In: year:2009
    In: number:6
    In: pages:795-804
    Description / Table of Contents: Heat flow anomalies provide critical information in active tectonic environments. The Gulf of Cadiz and adjacent areas are affected by the plate convergence between Africa and Europe, causing widespread deformation and faulting. Active thrust faults cause lateral movement and advection of heat that produces systematic variations in surface heat flow. In December 2003 new heat flow data were collected during the research vessel Sonne cruise SO175 in the Gulf of Cadiz over two sites of recent focused research activity: (i) the Gulf of Cadiz sedimentary prism and (ii) the Marques de Pombal escarpment. Both features have also been discussed as potential source areas of the Great Lisbon earthquake and tsunami of 1755. Background heat flow at the eastern terminus of the Horseshoe abyssal plain is about 5259 mW/m2. Over the Gulf of Cadiz prism, heat flow decreases from not, vert, similar57 mW/m2 to unusually low values of 45 mW/m2 roughly 120 km eastward. Such low values and the heat flow trend are typical for active thrusting, supporting the idea of an east-dipping thrust fault. Slip rates are 10 ± 5 mm per year, assuming that the fault dips at 2ʿ. A fault dipping at 5ʿ, however, would result into slip rates of 1.55 mm per year, suggesting that subduction has largely ceased. Based on seismic data, the Marques de Pombal fault is interpreted as part of an active fault system located not, vert, similar100 km westward of Cape San Vincente. Heat flow over the fault is affected by refraction of heat caused by the 1 km high escarpment. Thermal models suggest that the slip rate along the fault must either be small or shear stresses acting on the fault are rather high. With respect to other fault zones, however, it is reasonable to assume that the fault's slip rate is small.
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 0264-8172
    Language: English
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  • 2
    In: Geophysical journal international, Oxford : Oxford Univ. Press, 1958, 179(2009), 3, Seite 1265-1278, 1365-246X
    In: volume:179
    In: year:2009
    In: number:3
    In: pages:1265-1278
    Description / Table of Contents: The 1992 Nicaragua earthquake was a 'tsunami earthquake', which generated tsunamis disproportionately large for its surface wave magnitude Ms= 7.2 . Seismological studies and tsunami simulation indicated that the event was a slow earthquake, which occurred on the plate boundary between the subducting Cocos plate and the overriding Caribbean plate. We present a finite element model that enables us to estimate for the first time the temperature and inferred frictional conditions in the rupture area of a tsunami earthquake. Direct and indirect observations are used to constrain all model parameters, and surface heat-flux measurements provide independent information to verify the model results. Furthermore, we used a genetic algorithm to perform a sensitivity analysis of all model parameters and to define the spatial range of thermally defined updip limit of the seismogenic zone. The earthquake nucleated in the seismogenic zone at temperatures of ~150 °C and propagated updip towards the trench axis. The centroid or centre of mass of moment release was located in a region characterized by temperatures of ~50 °C. Thus, the rupture propagated through a region where plate motion is normally accommodated by aseismic creep. Our observations support a model in which tsunami earthquakes nucleate in the seismogenic zone near its updip limit. However, in such an environment coupled asperities are perhaps too small to cause large earthquakes. Seamounts, however, are abundant on the incoming Cocos plate. Therefore, in addition to temperature-dependent metamorphic induration of sediments, increased normal stress by seamount subduction may contribute to accumulate stress sufficiently large to release enough energy near the updip limit of the seismogenic zone to promote dynamic slip along a normally aseismic décollement all way to the ocean.
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 1365-246X
    Language: English
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  • 3
    In: Journal of seismology, Dordrecht [u.a.] : Springer Science + Business Media B.V, 1997, 13(2009), 4, Seite 543-559, 1573-157X
    In: volume:13
    In: year:2009
    In: number:4
    In: pages:543-559
    Description / Table of Contents: The construction of S-wave velocity models of marine sediments down to hundreds of meters below the seafloor is important in a number of disciplines. One of the most significant trends in marine geophysics is to use interface waves to estimate shallow shear velocities which play an important role in determining the shallow crustal structure. In marine settings, the waves trapped near the fluidsolid interface are called Scholte waves, and this is the subject of the study. In 1998, there were experiments on the Ninetyeast Ridge (Central Indian Ocean) to study the shallow seismic structure at the drilled site. The data were acquired by both ocean bottom seismometer and ocean bottom hydrophone. A new type of seafloor implosion sources has been used in this experiment, which successfully excited fast and high frequency (〉500 Hz) body waves and slow, intermediate frequency (〈20 Hz) Scholte waves. The fundamental and first higher mode Scholte waves have both been excited by the implosion source. Here, the Scholte waves are investigated with a full waveform modeling and a group velocity inversion approach. Shear wave velocities for the uppermost layers of the region are inferred and results from the different methods are compared. We find that the full waveform modeling is important to understand the intrinsic attenuation of the Scholte waves between 1 and 20 Hz. The modeling shows that the S-wave velocity varies from 195 to 350 m/s in the first 16 m of the uppermost layer. Depths levels of high S-wave impedance contrasts compare well to the layer depth derived from a P-wave analysis as well as from drilling data. As expected, the P- to S-wave velocity ratio is very high in the uppermost 16 m of the seafloor and the Poisson ratio is nearly 0.5. Depth levels of high S-wave impedance contrasts are comparable to the layer depth derived from drilling data.
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 1573-157X
    Language: English
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  • 4
    Keywords: Hochschulschrift ; Mittelatlantischer Rücken ; Lithosphäre ; Refraktionsseismik
    Type of Medium: Online Resource
    Pages: 1 Online-Ressource ( 168Seiten = 204MB) , Ill., graph. Darst.
    DDC: 550
    Language: English
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  • 5
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    Elsevier
    In:  Marine and Petroleum Geology, 26 . pp. 795-804.
    Publication Date: 2017-09-13
    Description: Heat flow anomalies provide critical information in active tectonic environments. The Gulf of Cadiz and adjacent areas are affected by the plate convergence between Africa and Europe, causing widespread deformation and faulting. Active thrust faults cause lateral movement and advection of heat that produces systematic variations in surface heat flow. In December 2003 new heat flow data were collected during the research vessel Sonne cruise SO175 in the Gulf of Cadiz over two sites of recent focused research activity: (i) the Gulf of Cadiz sedimentary prism and (ii) the Marques de Pombal escarpment. Both features have also been discussed as potential source areas of the Great Lisbon earthquake and tsunami of 1755. Background heat flow at the eastern terminus of the Horseshoe abyssal plain is about 52–59 mW/m2. Over the Gulf of Cadiz prism, heat flow decreases from ∼57 mW/m2 to unusually low values of 45 mW/m2 roughly 120 km eastward. Such low values and the heat flow trend are typical for active thrusting, supporting the idea of an east-dipping thrust fault. Slip rates are 10 ± 5 mm per year, assuming that the fault dips at 2°. A fault dipping at 5°, however, would result into slip rates of 1.5–5 mm per year, suggesting that subduction has largely ceased. Based on seismic data, the Marques de Pombal fault is interpreted as part of an active fault system located ∼100 km westward of Cape San Vincente. Heat flow over the fault is affected by refraction of heat caused by the 1 km high escarpment. Thermal models suggest that the slip rate along the fault must either be small or shear stresses acting on the fault are rather high. With respect to other fault zones, however, it is reasonable to assume that the fault's slip rate is small.
    Type: Article , PeerReviewed
    Format: text
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  • 6
    Publication Date: 2012-02-23
    Type: Conference or Workshop Item , NonPeerReviewed
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  • 7
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    In:  [Talk] In: 69. Jahrestagung der Deutschen Geophysikalischen Gesellschaft (DGG), 23.03.-26.03.2009, Kiel . 69. Jahrestagung der Deutschen Geophysikalischen Gesellschaft in Kiel : 23. - 26. März 2009 ; pp. 15-16 .
    Publication Date: 2012-02-23
    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:  [Other] In: 69. Jahrestagung der Deutschen Geophysikalischen Gesellschaft (DGG), 23.03.-26.03.2009, Kiel . 69. jahrestagung der Deutschen Geophysikalischen Gesellschaft in Kiel : 23.-26. März 2009 ; p. 36 .
    Publication Date: 2012-02-23
    Type: Conference or Workshop Item , NonPeerReviewed
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  • 10
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    In:  [Other] In: 69. Jahrestagung der Deutschen Geophysikalischen Gellschaft (DGG), 23.03.-26.03.2009, Kiel . 69. Jahrestagung der Deutschen Geophysikalischen Gellschaft in Kiel : 23.-26. März 2009 ; p. 30 .
    Publication Date: 2012-02-23
    Type: Conference or Workshop Item , NonPeerReviewed
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