Synoptic View of Lithospheric S-Wave Velocity Structure in the Southern United States: A Comparison of 3D Seismic Tomographic Models

Q1 Earth and Planetary Sciences GSA Today Pub Date : 2019-07-01 DOI:10.1130/GSATG387A.1
A. Netto, J. Pulliam, P. Persaud
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The spatial extent of smaller-scale tectonic features, such as the Sabine Uplift and Wiggins block, remains poorly resolved. An inverse relationship between crustal thickness and Bouguer gravity across the continental margin is observed. This model comparison highlights the need for additional P-wave tomography studies and targeted, higher density station deployments to better constrain tectonic features. INTRODUCTION The southern U.S. margin (Fig. 1) ranges from the stable Laurentia craton beneath Oklahoma to a stretched and thinned passive margin to oceanic lithosphere in the deep Gulf of Mexico, recording within it a geologic history that includes two complete Wilson cycles (Thomas, 2006). Due to its extensive hydrocarbon reserves, the southern U.S. has been the focus of intensive seismic exploration. However, until recently, studies of its deep structure trailed those of other U.S. continental margins. The result is that the tectonomagmatic evolution of the southern U.S. margin remains poorly understood. The primary contributing factors to this status quo are (1) the presence of a thick sediment cover that obscures crustal structure through most of the region, (2) the paucity of significant local seismicity, and, until recently, (3) sparse seismic instrumentation in the region. Earthscope’s USArray temporarily densified the set of broadband seismographs available for studies of the region’s lithosphere (http://www.usarray.org/ researchers/obs/transportable). Approximately 435 stations occupied a total of 1830 locations in the continental U.S., for two years each, at a nominal spacing of 70 km. In USArray’s wake, there has been a surge in the number of continental-scale tomographic studies presenting snapshots of the compressional and shear wave velocities of the region’s crust and upper mantle. 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引用次数: 3

Abstract

The southern U.S. continental margin records a history spanning ca. 1.2 Ga, including two Wilson cycles. However, due to a thick sediment cover, the paucity of significant local seismicity, and, until recently, sparse instrumentation, details of this passive margin’s tectonomagmatic evolution remain disputed. This paper compares recent S-wave tomography and crustal thickness models based on USArray data to help establish a framework for geodynamic interpretation. Large-scale patterns of crustal velocity anomalies, corresponding to major regional features such as the Ouachita orogenic front and the Precambrian margin, are generally consistent between the models. The spatial extent of smaller-scale tectonic features, such as the Sabine Uplift and Wiggins block, remains poorly resolved. An inverse relationship between crustal thickness and Bouguer gravity across the continental margin is observed. This model comparison highlights the need for additional P-wave tomography studies and targeted, higher density station deployments to better constrain tectonic features. INTRODUCTION The southern U.S. margin (Fig. 1) ranges from the stable Laurentia craton beneath Oklahoma to a stretched and thinned passive margin to oceanic lithosphere in the deep Gulf of Mexico, recording within it a geologic history that includes two complete Wilson cycles (Thomas, 2006). Due to its extensive hydrocarbon reserves, the southern U.S. has been the focus of intensive seismic exploration. However, until recently, studies of its deep structure trailed those of other U.S. continental margins. The result is that the tectonomagmatic evolution of the southern U.S. margin remains poorly understood. The primary contributing factors to this status quo are (1) the presence of a thick sediment cover that obscures crustal structure through most of the region, (2) the paucity of significant local seismicity, and, until recently, (3) sparse seismic instrumentation in the region. Earthscope’s USArray temporarily densified the set of broadband seismographs available for studies of the region’s lithosphere (http://www.usarray.org/ researchers/obs/transportable). Approximately 435 stations occupied a total of 1830 locations in the continental U.S., for two years each, at a nominal spacing of 70 km. In USArray’s wake, there has been a surge in the number of continental-scale tomographic studies presenting snapshots of the compressional and shear wave velocities of the region’s crust and upper mantle. Although the volume of seismic data available for studies of the region has increased dramatically and sampling of the subsurface has improved as well, the presence of a thick layer of sediments and relatively low levels of seismicity (with the exception of Oklahoma) continue to challenge efforts to image the lithosphere. The collection of models for the southern U.S. region represents the state-of-theart of seismic tomography: a broad range of approaches, the inclusion of various types of data, and different choices of solution schemes. These seismic velocity models can be used to study the mineralogical, compositional, and thermal state of the current crust and upper mantle, and thereby provide critical constraints on geodynamic models, as well as serving as a foundation to launch further investigations. They also showcase the various techniques and innovations of seismic tomography. But, first, robust tectonic features must be identified. Well-constrained features should appear consistently across models. Differences between models could be due to (1) types of data incorporated, such as body wave arrival times, surface wave dispersion, receiver functions, or combinations of two or more data types; (2) measurement techniques employed; (3) the theoretical basis of the forward calculation, such as ray theory versus finite difference versus finite frequency; (4) the initial model and parameterization used; (5) regularization choices (“damping” and “smoothing” schemes and parameter values); and (6) inversion methods, such as gradient-based local minimization versus global optimization techniques. The purpose of this study is to provide a systematic analysis of similarities and differences between recent shear wave tomographic models with respect to the lithospheric structure of the southern U.S. continental margin. Similar comparisons have been conducted for the western U.S. by Becker (2012) and Pavlis et al. (2012).
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美国南部岩石圈s波速度结构的概观:三维地震层析模型的比较
美国南部大陆边缘的历史跨度约为1.2 Ga,包括两个威尔逊旋回。然而,由于沉积物覆盖层厚,缺乏显著的局部地震活动,以及直到最近仪器稀少,这一被动边缘构造岩浆演化的细节仍然存在争议。本文比较了最近的S波层析成像和基于USArray数据的地壳厚度模型,以帮助建立地球动力学解释的框架。与Ouachita造山带前缘和前寒武纪边缘等主要区域特征相对应的地壳速度异常的大规模模式在模型之间基本一致。较小规模构造特征的空间范围,如Sabine隆起和Wiggins地块,仍然没有得到很好的解决。在整个大陆边缘观察到地壳厚度和布格重力之间的反比关系。这种模型比较突出了额外的P波层析成像研究和有针对性的高密度台站部署的必要性,以更好地约束构造特征。引言美国南部边缘(图1)从俄克拉荷马州下方稳定的劳伦克拉通到墨西哥湾深处海洋岩石圈的拉伸和变薄被动边缘,记录了包括两个完整威尔逊旋回的地质历史(Thomas,2006)。由于其广泛的碳氢化合物储量,美国南部一直是密集地震勘探的重点。然而,直到最近,对其深层结构的研究还落后于对美国其他大陆边缘的研究。其结果是,人们对美国南部边缘的构造岩浆演化仍知之甚少。造成这种现状的主要因素是:(1)该地区大部分地区存在厚厚的沉积物覆盖层,掩盖了地壳结构,(2)缺乏显著的局部地震活动,以及直到最近,(3)该地区地震仪器稀少。Earthscope的USArray暂时加密了可用于研究该地区岩石圈的宽带地震仪(http://www.usarray.org/研究人员/obs/可运输)。大约435个台站在美国大陆总共占据了1830个地点,每个台站为期两年,标称间距为70公里。在USArray的尾流中,提供该地区地壳和上地幔压缩和剪切波速快照的大陆级断层摄影研究数量激增。尽管可用于该地区研究的地震数据量大幅增加,地下采样也有所改善,但厚厚的沉积物层和相对较低的地震活动水平(俄克拉荷马州除外)继续挑战岩石圈成像工作。美国南部地区的模型集合代表了地震层析成像的最新状态:广泛的方法,包括各种类型的数据,以及不同的解决方案选择。这些地震速度模型可用于研究当前地壳和上地幔的矿物学、成分和热状态,从而为地球动力学模型提供关键约束,并作为开展进一步研究的基础。他们还展示了地震层析成像的各种技术和创新。但是,首先,必须确定坚固的构造特征。受良好约束的特征应在模型中一致显示。模型之间的差异可能是由于(1)包含的数据类型,如体波到达时间、表面波色散、接收器功能或两种或多种数据类型的组合;(2) 采用的测量技术;(3) 正演计算的理论基础,如射线理论与有限差分法与有限频率法;(4) 使用的初始模型和参数化;(5) 正则化选择(“阻尼”和“平滑”方案和参数值);以及(6)反演方法,例如基于梯度的局部最小化与全局优化技术。本研究的目的是系统分析美国南部大陆边缘岩石圈结构的近期剪切波层析成像模型之间的异同。Becker(2012)和Pavlis等人(2012)对美国西部进行了类似的比较。
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来源期刊
GSA Today
GSA Today Earth and Planetary Sciences-Geology
CiteScore
4.90
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20
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