首页> 外文期刊>Tectonophysics: International Journal of Geotectonics and the Geology and Physics of the Interior of the Earth >Crustal structure beneath Tierra del Fuego, Argentina, inferred from seismic P-wave receiver functions and ambient noise autocorrelations
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Crustal structure beneath Tierra del Fuego, Argentina, inferred from seismic P-wave receiver functions and ambient noise autocorrelations

机译:在阿根廷的地震P波接收器功能和环境噪声自相关,地壳结构下面的地壳结构。推断

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摘要

We investigate the structure of the crust beneath the main island of Tierra del Fuego through a teleseismic receiver function analysis and ambient seismic noise autocorrelation using data of four available broad-band stations. The area is situated in a remote region of southern Argentina where the interaction between the South American and Scotia plates define the Magallanes-Fagnano Fault System. Crustal thickness, Vp/Vs ratios and S-wave velocity models were estimated using the H-k stacking method and the inversion of receiver functions with the Neighbourhood Algorithm. Furthermore, we applied an ambient seismic noise autocorrelation procedure to identify PmP Moho reflections at all stations. The three methods provide consistent estimates for the crustal thickness which ranges from about 24.5 km in the northern part of the Island to about 39.2 km in the south. The lowest and highest values of S-wave velocity found, in the most superficial layers of the crust, correlate with the presence of Tertiary and upper Cretacic sediments in the north and with older geological units composed by more consolidated lithologies in the south, respectively. Despite the diverse geological and tectonic settings present, our results do not change significantly for different parameters or subsidiary data sets, i.e., showing the robustness of our models which likely represent closely the local structure beneath the Island. This area is considered a very seismically active one and its crustal structure has been little explored demonstrating the importance of having new models and the necessity to increase the station coverage to allow a more detailed study of the region. Furthermore, the models presented here provide better constraints on the crustal structure, and will facilitate studies of the regional seismicity that can improve our understanding of the seismic hazard posed by earthquakes such as the magnitude 7.5 and 7.8 events that occurred in 1949.
机译:我们正在使用四个可用的宽带站的数据来调查Tierra Del Fuego主岛主岛下面的地壳的结构。该地区位于阿根廷南部的偏远地区,南美和斯科蒂亚平板之间的互动定义了Magallanes-Fagnano故障系统。使用H-K堆叠方法估计地壳厚度,VP / VS比率和S波速度模型以及与邻域算法的接收器功能的反转。此外,我们应用了环境地震噪声自相关过程,以识别所有站的PMP Moho反射。这三种方法为岛屿北部约24.5公里的地壳厚度提供了一致的估计,南部约为39.2公里。在地壳的最浅表层中发现的S波速度最低和最高值与北方的北方和上齐齐提比亚的存在相关,分别与南部更多综合岩性组成的旧地质单位。尽管存在多样化的地质和构造环境,但我们的结果对于不同的参数或子公司数据集,即,展示了我们模型的稳健性,这可能不会显着变化,这可能是岛下方的局部结构。该地区被认为是一个非常地震活动的一个,其地壳结构一直很少探索,证明具有新模型的重要性和增加站覆盖范围的必要性,以允许对该地区更详细地研究。此外,这里提出的模型在地壳结构上提供了更好的限制,并促进了可以改善我们对1949年发生的幅度7.5和7.8事件所构成的地震危害的区域地震性的研究。

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