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  • 1
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 269(2008), 1/2, Seite 41-55, 1385-013X
    In: volume:269
    In: year:2008
    In: number:1/2
    In: pages:41-55
    In: extent:15
    Description / Table of Contents: We examine the micro-earthquake seismicity recorded by two temporary arrays of ocean bottom seismometers on the outer rise offshore southern Chile on young oceanic plate of ages 14 Ma and 6 Ma, respectively. The arrays were in operation from December 2004January 2005 and consisted of 17 instruments and 12 instruments, respectively. Approximately 10 locatable events per day were recorded by each of the arrays. The catalogue, which is complete for magnitudes above 1.21.5, is characterized by a high b value, i.e., a high ratio of small to large events, and the data set is remarkable in that a large proportion of the events form clusters whose members show a high degree of waveform similarity. The largest cluster thus identified consisted of 27 similar events (average inter-event correlation coefficient N0.8 for a 9.5 s window), and waveform similarity persists far into the coda. Inter-event spacing is irregular, but very short waiting times of a few minutes are far more common than expected from a Poisson distribution. Seismicity with these features (high b value, large number of similar events with short waiting times) is typical of swarm activity, which, based on empirical evidence and theoretical considerations, is generally thought to be driven by fluid pressure variations. Because no pronounced outer rise bulge exists on the very young plate in the study region, it is unlikely that melt is accessible from decompression melting or opening of cracks. A fluid source related to processes at the nearby ridge is conceivable for the younger segment but less likely for the older one. We infer that the fluid source could be seawater, which enters through fractures in the crust. Most of the similarearthquake clusters are within the crust, but some of them locate significantly below the Moho. If our interpretation is correct, this implies that water is present within the mantle. Hydration of the mantle is also indicated by a decrease of Pn velocities below the outer rise seen on a refraction profile through one of the arrays [Contreras-Reyes, E., Grevemeyer, I., Flueh, E.R., Scherwath, M., Heesemann, M., 2007. Alteration of the subducting oceanic lithosphere at the southern central Chile trench-outer rise. Geochem., Geophys. Geosyst. 8, Q07003.]. The deepest events within the array on the 6 Ma old plate occur where the temperature reaches 500600 ʿC, consistent with the value observed for large intraplate earthquakes within the mantle (650 ʿC), suggesting that the maximum temperature at which these fluid-mediated micro-earthquakes can occur is similar or identical to that of large earthquakes.
    Type of Medium: Online Resource
    Pages: 15 , graph. Darst., Kt
    ISSN: 1385-013X
    Language: English
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  • 2
    Publication Date: 2014-12-16
    Description: On 27 February 2010 the Mw 8.8 Maule earthquake in Central Chile ruptured a well known seismic gap, which last broke in 1835. Shortly after the mainshock Chilean agencies (UC Santiago, UC Concepción) and the international seismological community (USA (IRIS), France (IPGP), UK (University of Liverpool), Germany (GFZ)) installed a total of 142 portable seismic landstations stations along the whole rupture zone in order to capture the aftershock activity. Additionally a network of 30 ocean bottom seismometers was deployed (IFM Geomar) in the northern portion of the rupture area for a three month period between 20 September 2010 and 25 December 2010. We present first results from local earthquake tomography based on arrival times from automatic detection algorithms and picking engines which are calibrated with manually picked events. The Vp and Vp/Vs velocity models will better illuminate the structure of the forearc including the downgoing slab, the sedimentary basins and the volcanic arc down to depths of 75 km. The 2D and 3D velocity models cover the northern part of the rupture Maule 2010 rupture zone between 33 ° and 36 °S. This region is characterized by pronounced crustal aftershock activity which started after a strong aftershock doublet (Mw=6.9) on 11 March 2010 near the city of Pichilemu (~34.5 °S) in the overriding plate. This pronounced cluster of crustal seismicity close to the city of Pichilemu will be the focus area with smaller node spacing of the velocity model.
    Type: Conference or Workshop Item , NonPeerReviewed
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  • 3
    Publication Date: 2013-10-22
    Type: Conference or Workshop Item , NonPeerReviewed
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