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Dislocation creep near the frictional-viscous transition in blueschist: experimental constraints 蓝晶岩摩擦粘性转变附近的位错蠕变:实验约束
IF 3.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-05-29 DOI: 10.5194/egusphere-2024-1507
Lonnie Justin Hufford, Leif Tokle, Whitney Maria Behr, Luiz Grafula Morales, Claudio Madonna
Abstract. Mafic oceanic crustal rocks at blueschist facies conditions are an important rheological component of subducting slabs and the interface at subduction plate boundaries. However, the mechanical properties and deformation mechanisms of glaucophane, a rheologically-controlling sodic amphibole in blueschists, are poorly constrained. To investigate its mechanical and microstructural properties, we conducted general shear constant rate and strain rate stepping experiments on glaucophane aggregates using a Griggs apparatus at temperatures of 700–750 °C, shear strain rates of ~3x10-6 to 9x10-5 s-1, varying grain sizes, and a confining pressure of ~1.0 GPa. The constant rate experiments show an initial stage of grain-size-dependent strain hardening followed by weakening associated with brittle slip along cleavage planes, kink-band development, cataclasis resulting in a fine-grained matrix, and dislocation glide. These experiments evolved to a steady-state stress that did not depend on starting grain size, showing evidence for subgrain development and dynamic recrystallization by bulge nucleation, interpreted to reflect dislocation creep with limited recovery by climb. The mechanical behavior and microstructures of glaucophane in our experiments are consistent with experiments on other low-symmetry minerals as well as microstructural observations from natural blueschists. The strain rate stepping experiments were used to develop a dislocation creep flow law for glaucophane with values of A = 2.23 x 105 MPa-n s-1, n = 3, and Q = 341 ± 37 kJ/mol. A deformation mechanism map comparing our dislocation creep flow law to an existing flow law for blueschist diffusion creep indicates dislocation creep should activate at lower temperatures, higher stresses and larger diffusion lengthscales. Viscosities predicted by our flow law for a typical subduction strain rate of 1 x 10-12 s-1 lie between quartz and eclogite dislocation creep for the blueschist stability field, implying that mafic oceanic crustal rocks remain strong relative to quartz-rich metasediments all along the subduction interface.
摘要处于蓝晶岩岩相条件下的岩浆大洋地壳岩石是俯冲板块和俯冲板块边界界面的重要流变成分。然而,蓝晶岩中的一种流变控制性钠闪石--琉璃玢岩的力学性质和变形机制却鲜为人知。为了研究它的机械和微观结构特性,我们使用格里格斯仪器在温度为 700-750 °C、剪切应变速率为 ~3x10-6 至 9x10-5 s-1、晶粒大小不同和约束压力为 ~1.0 GPa 的条件下,对玻璃钙钛矿聚集体进行了一般剪切恒定速率和应变速率阶跃实验。恒定应变速率实验表明,在晶粒尺寸相关应变硬化的初始阶段,会出现与沿劈裂面的脆性滑移、扭结带发展、导致细晶粒基体的催化和位错滑移相关的削弱。这些实验发展到了不依赖于起始晶粒大小的稳态应力,显示了亚晶粒发育和隆起成核动态再结晶的证据,可以解释为反映了位错蠕变和有限的爬升恢复。在我们的实验中,玻璃釉的机械行为和微观结构与其他低对称性矿物的实验以及天然蓝晶岩的微观结构观察结果一致。通过应变速率阶跃实验,我们得出了玻璃釉的位错蠕变流动规律:A = 2.23 x 105 MPa-n s-1、n = 3、Q = 341 ± 37 kJ/mol。将我们的位错蠕变流动定律与现有的蓝晶扩散蠕变流动定律进行比较的变形机制图表明,位错蠕变应在较低温度、较高应力和较大扩散长度尺度下启动。在典型的俯冲应变速率为1 x 10-12 s-1时,我们的流动定律预测的粘度介于蓝晶岩稳定场的石英和斜长岩位错蠕变之间,这意味着在整个俯冲界面上,相对于富含石英的玄武岩,黑云母大洋型地壳岩石仍然很坚固。
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引用次数: 0
On the role of trans-lithospheric faults in the long-term seismotectonic segmentation of active margins: a case study in the Andes 跨岩石圈断层在活动边缘长期地震构造分割中的作用:安第斯山脉案例研究
IF 3.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-05-27 DOI: 10.5194/egusphere-2024-1338
Gonzalo Yanez, Jose Piquer, Orlando Rivera
Abstract. Plate coupling play a fundamental role in the way in which seismic energy is released during the seismic cycle. This process includes quasi-instantaneous release during megathrust earthquakes and long-term creep. Both mechanisms can coexist in a given subducting margin, defining a seismotectonic segmentation in which seismically active segments are separated by zones in which ruptures stop, classified for simplicity as asperities and barrier, respectively. The spatiotemporal stability of this segmentation has been a matter of debate in the seismological community for decades. At this regard, we explore in this paper the potential role of the interaction between geological heterogeneities in the overriding plate and fluids released from the subducting slab towards the subduction channel. As a case study, we take the convergence between the Nazca and South American plates between 18°–40° S, given its relatively simple convergence style and the availability of a high-quality instrumental and historical record. We postulate that trans-lithospheric faults striking at a high angle with respect to the trench behave as large fluid sinks that create the appropriate conditions for the development of barriers and promote the growth of highly coupled asperity domains in their periphery. We tested this hypothesis against key short- and long-term observations in the study area, obtaining consistent results. If the spatial distribution of asperities is controlled by the geology of the overriding plate, seismic risk assessment could be established with better confidence.
摘要板块耦合对地震周期中地震能量的释放方式起着根本性的作用。这一过程包括大地壳地震时的准瞬时释放和长期蠕变。在特定的俯冲边缘,这两种机制可能同时存在,从而形成地震构造分段,其中地震活动段被断裂停止区隔开,为简单起见,断裂停止区分别被划分为尖顶区和屏障区。几十年来,地震学界一直在争论这种分段的时空稳定性。为此,我们在本文中探讨了凌覆板块中的地质异质性与俯冲板块向俯冲通道释放的流体之间相互作用的潜在作用。我们以南纬18°-40°之间的纳斯卡板块和南美板块的汇聚为例进行研究,因为其汇聚方式相对简单,而且有高质量的仪器和历史记录。我们推测,与海沟呈高角度的跨岩石圈断层是一个大的流体汇,它为障碍物的发展创造了适当的条件,并促进了其外围高度耦合的尖顶域的生长。我们根据研究区域的主要短期和长期观测结果对这一假设进行了检验,得到了一致的结果。如果非主流的空间分布受到凌空板块地质的控制,那么地震风险评估就能更有把握地进行。
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引用次数: 0
Revised conceptual model of the Solfatara magmatic-hydrothermal system (Campi Flegrei, Italy), time changes during the last 40 years, and prediction of future scenarios 索尔法塔拉岩浆-热液系统(意大利坎皮弗莱格雷)的修订概念模型、过去 40 年的时间变化以及未来情景预测
IF 3.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-05-22 DOI: 10.5194/egusphere-2024-1306
Luigi Marini, Claudia Principe, Matteo Lelli
Abstract. We revised the conceptual model of the Solfatara magmatic-hydrothermal system based on the results of new gas-geoindicators (Marini et al., 2022) and the available geological, volcanological, and geophysical information from surface surveys and deep geothermal wells. Using the new gas-geoindicators, we monitored the temperature and total fluid pressure over a time interval of ~40 years: (i) in the shallow reservoir (0.25–0.45 km depth), where CO equilibrates; (ii) in the intermediate reservoir (2.7–4.0 km depth), where CH4 attains equilibrium; (iii) in the deep reservoir (6.5–7.5 km depth), where H2S achieves equilibrium. From 1983 to 2022, the temperature and total fluid pressure of the shallow reservoir did not depart significantly from ~220 °C and ~25 bar, whereas remarkable, progressive increments in temperature and total fluid pressure occurred in the intermediate and deep reservoirs, with peak values of 590–620 °C and 1200–1400 bar in the intermediate reservoir and 1010–1040 °C and 3000–3200 bar in the deep reservoir, in 2020. The revised conceptual model allowed us to explain the evolution of: (a) pressurization-depressurization in the intermediate reservoir, acting as the “engine” of bradyseism, (b) time changes of total fluid pressure in the deep reservoir, working as the “on-off switch” of magmatic degassing. We also used the revised conceptual model to predict possible future scenarios in the lack of external factors.
摘要我们根据新的气体地质指示剂(Marini 等人,2022 年)的结果以及地表勘测和深层地热井提供的现有地质、火山和地球物理信息,修订了索尔法塔拉岩浆-热液系统的概念模型。利用新的气体地质指标,我们监测了约 40 年时间间隔内的温度和总流体压力:(i) 浅层储层(0.25-0.45 千米深),CO 在此达到平衡;(ii) 中层储层(2.7-4.0 千米深),CH4 在此达到平衡;(iii) 深层储层(6.5-7.5 千米深),H2S 在此达到平衡。从 1983 年到 2022 年,浅层储层的温度和总流体压力没有明显偏离 ~220 °C 和 ~25 bar,而中层和深层储层的温度和总流体压力出现了显著的渐进式增长,到 2020 年,中层储层的峰值为 590-620 °C 和 1200-1400 bar,深层储层的峰值为 1010-1040 °C 和 3000-3200 bar。修订后的概念模型使我们能够解释以下方面的演变:(a) 中间储层的增压-减压,作为缓震的 "发动机";(b) 深层储层总流体压力的时间变化,作为岩浆脱气的 "开关"。我们还利用修订后的概念模型预测了在缺乏外部因素的情况下未来可能出现的情况。
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引用次数: 0
Coda-derived source properties estimated using local earthquakes in the Sea of Marmara, Türkiye 利用土尔其马尔马拉海当地地震估算的正弦源特性
IF 3.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-05-15 DOI: 10.5194/egusphere-2024-721
Berkan Özkan, Tuna Eken, Peter Gaebler, Tuncay Taymaz
Abstract. Accurate estimates of the moment magnitude of earthquakes that physically measures the earthquake source energy are crucial for improving our understanding of seismic hazards in regions prone to tectonic activity. To address this need, a method involving coda wave modelling was employed to estimate the moment magnitudes of earthquakes in the Sea of Marmara. This approach enabled to model the source displacement spectrum of 303 local earthquakes recorded at 49 seismic stations between 2018 and 2020 in this region. The coda wave traces of individual events were inverted across twelve frequency ranges between 0.3 and 16 Hz. The resultant coda-derived moment magnitudes were found to be in good accordance with the standard local magnitude estimates. However, the notable move-out between local magnitude and coda-derived moment magnitude estimates for smaller earthquakes less than a magnitude of 3.5 likely occurs due to potential biases arising from incorrect assumptions for anelastic attenuation and the finite sampling intervals of seismic recordings. Scaling relations between the total radiated energy and seismic moment imply a nonself-similar behaviour for the earthquakes in the Sea of Marmara. Our findings suggest that larger earthquakes in the Sea of Marmara exhibit distinct rupture dynamics compared to smaller ones, resulting in a more efficient release of seismic energy. In conclusion, here we introduce an empirical relationship devised from the scatter between local magnitude and coda-derived moment magnitude estimates.
摘要对地震力矩震级的精确估算能够物理测量地震源能量,这对于提高我们对构造活动多发地区地震危害的认识至关重要。为了满足这一需求,我们采用了一种涉及尾波建模的方法来估算马尔马拉海地震的矩震级。这种方法能够对 2018 年至 2020 年期间该地区 49 个地震台站记录的 303 次当地地震的震源位移谱进行建模。在 0.3 至 16 Hz 的 12 个频率范围内,对单个事件的尾波轨迹进行了反演。结果发现,尾波推导出的矩震级与当地标准震级估计值十分吻合。然而,对于震级小于 3.5 级的较小地震,当地震级与根据尾波推导的矩震级估计值之间存在明显偏差,这可能是由于对无弹性衰减的不正确假设和地震记录的有限采样间隔造成的潜在偏差。总辐射能量和地震力矩之间的比例关系意味着马尔马拉海的地震具有非自相似性。我们的研究结果表明,马尔马拉海较大的地震与较小的地震相比,表现出不同的破裂动态,从而更有效地释放地震能量。总之,我们在此介绍一种经验关系,该关系是根据当地震级与尾波推导的矩震级估计值之间的散差设计的。
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引用次数: 0
Importance of basement faulting and salt decoupling for the structural evolution of the Fars Arc, Zagros fold-and-thrust belt: A numerical modeling approach 基底断层和盐分脱钩对扎格罗斯褶皱-推力带法尔斯弧的结构演变的重要性:数值建模方法
IF 3.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-05-14 DOI: 10.5194/egusphere-2024-1123
Fatemeh Gomar, Jonas Bruno Ruh, Mahdi Najafi, Farhad Sobouti
Abstract. Understanding the tectonic evolution and crustal-scale structure of fold-thrust belts is crucial for exploring geological resources and evaluating seismic hazards. We conducted a series of finite-difference two-dimensional thermo-mechanical numerical models with visco-elasto-plastic/brittle rheology to decipher how the interaction of inherited basement faults and salt décollement levels control the deformation process and structural style of the Fars Arc in the Zagros fold -thrust belt, during tectonic inversion. Results indicate that initial rifting is controlled by the geometry of inherited faults. During the convergence phase, fold-and-thrust belts display folding at two scales: large wavelength folds induced by basement deformation in the form of fault-propagation faults, and small wavelength folds and thrust systems emerge above the salt layer as detachment folds. Reactivated faults can serve as pathways for stress transfer, resulting in the emergence of new faults and thus seismic activity. The tectonic events in orogenic belts like the Zagros do not adhere to a fixed pattern; they are shaped by factors such as the properties of basement rocks and the orientation of faults. Shallow earthquakes predominantly occur along décollement anticlines, while deeper and larger ones are associated with basement faults. Additionally, we observe variations in resistance to deformation based on salt rheology and fault geometry, with listric faults minimizing resistance. The degree of basement involvement in deformation directly influences the model's resistance, with greater involvement facilitating easier deformation. Our results showing the temporal-spatial relationship between thin- and thick-skinned tectonics can work as an analogue for similar orogenic belts worldwide, such as Taiwan, the Pyrenees, the Alps, the Appalachians, and the Kopet Dagh.
摘要。了解褶皱推覆带的构造演化和地壳尺度结构对于勘探地质资源和评估地震灾害至关重要。我们采用粘弹性/脆性流变学方法,建立了一系列有限差分二维热力-力学数值模型,以破解在构造反演过程中,基底继承断层和盐溶层的相互作用如何控制扎格罗斯褶皱-推覆带法尔斯弧的变形过程和构造样式。研究结果表明,最初的断裂由继承断层的几何形状控制。在汇聚阶段,褶皱-推力带显示出两种规模的褶皱:由基底变形诱发的大波长褶皱以断层扩展断层的形式出现,而小波长褶皱和推力系统则以脱离褶皱的形式出现在盐层之上。重新激活的断层可作为应力传递的途径,导致新断层的出现,从而引起地震活动。扎格罗斯等造山带的构造活动并不固定,而是受基底岩石性质和断层走向等因素的影响。浅层地震主要沿着地壳反褶发生,而较深和较大的地震则与基底断层有关。此外,我们还观察到根据盐的流变性和断层的几何形状,变形阻力也会发生变化,其中列状断层的阻力最小。基底参与变形的程度直接影响模型的阻力,参与程度越高,变形越容易。我们的研究结果表明了薄皮构造和厚皮构造之间的时空关系,可以作为全球类似造山带的类比,如台湾、比利牛斯山脉、阿尔卑斯山脉、阿巴拉契亚山脉和科佩特达赫山脉。
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引用次数: 0
On the impact of true polar wander on heat flux patterns at the core–mantle boundary 真正的极地漫游对地核-地幔边界热通量模式的影响
IF 3.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-05-14 DOI: 10.5194/se-15-617-2024
Thomas Frasson, Stéphane Labrosse, Henri-Claude Nataf, Nicolas Coltice, Nicolas Flament
Abstract. The heat flux across the core–mantle boundary (CMB) is a fundamental variable for Earth evolution and internal dynamics. Seismic tomography provides access to seismic heterogeneities in the lower mantle, which can be related to present-day thermal heterogeneities. Alternatively, mantle convection models can be used to either infer past CMB heat flux or to produce statistically realistic CMB heat flux patterns in self-consistent models. Mantle dynamics modifies the inertia tensor of the Earth, which implies a rotation of the Earth with respect to its spin axis, a phenomenon called true polar wander (TPW). This rotation must be taken into account to link the dynamics of the mantle to the dynamics of the core. In this study, we explore the impact of TPW on the CMB heat flux over long timescales (∼1 Gyr) using two recently published mantle convection models: one model driven by a plate reconstruction and a second that self-consistently produces a plate-like behaviour. We compute the geoid in both models to correct for TPW. In the plate-driven model, we compute a total geoid and a geoid in which lateral variations of viscosity and density are suppressed above 350 km depth. An alternative to TPW correction is used for the plate-driven model by simply repositioning the model in the original paleomagnetic reference frame of the plate reconstruction. The average TPW rates range between 0.4 and 1.8° Myr−1, but peaks up to 10° Myr−1 are observed. We find that in the plate-driven mantle convection model used in this study, the maximum inertia axis produced by the model does not show a long-term consistency with the position of the magnetic dipole inferred from paleomagnetism. TPW plays an important role in redistributing the CMB heat flux, notably at short timescales (≤10 Myr). Those rapid variations modify the latitudinal distribution of the CMB heat flux, which is known to affect the stability of the magnetic dipole in geodynamo simulations. A principal component analysis (PCA) is computed to obtain the dominant CMB heat flux pattern in the different cases. These heat flux patterns are representative of the mantle convection cases studied here and can be used as boundary conditions for geodynamo models.
摘要穿过地核-地幔边界(CMB)的热通量是地球演化和内部动力学的一个基本变量。通过地震层析成像可以获得下地幔的地震异质性,并将其与当今的热异质性联系起来。另外,地幔对流模型可用于推断过去的 CMB 热通量,或在自洽模型中产生统计上真实的 CMB 热通量模式。地幔动力学改变了地球的惯性张量,这意味着地球相对于其自旋轴的旋转,这种现象被称为真正的极地漂移(TPW)。要将地幔动力学与地核动力学联系起来,就必须考虑到这种旋转。在这项研究中,我们利用最近发表的两个地幔对流模型(一个是由板块重建驱动的模型,另一个是自洽地产生类似板块行为的模型),探讨了 TPW 在长时间尺度(∼1 Gyr)上对 CMB 热通量的影响。我们计算了两个模型的大地水准面,以校正TPW。在板块驱动模型中,我们计算了总大地水准面和大地水准面,其中粘度和密度的横向变化在深度 350 公里以上被抑制。在板块驱动模型中,我们采用了另一种方法来校正 TPW,即在板块重建的原始古地磁参考框架内重新定位模型。平均 TPW 率介于 0.4 至 1.8° Myr-1 之间,但观测到的峰值可达 10° Myr-1。我们发现,在本研究使用的板块驱动地幔对流模型中,模型产生的最大惯性轴与古地磁推断的磁偶极子位置并不长期一致。TPW在重新分配CMB热通量方面起着重要作用,尤其是在短时标(≤10 Myr)。这些快速变化改变了 CMB 热通量的纬度分布,众所周知,这会影响地球动力模拟中磁偶极子的稳定性。通过计算主成分分析(PCA),可以得到不同情况下的主要 CMB 热通量模式。这些热通量模式代表了本文研究的地幔对流情况,可用作地球动力模型的边界条件。
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引用次数: 0
Multiscalar 3D temporal structural characterisation of Smøla island, mid-Norwegian passive margin: an analogue for unravelling the tectonic history of offshore basement highs 挪威被动边缘中部斯莫拉岛的多尺度三维时间结构特征:揭示近海基底高地构造历史的类比研究
IF 3.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-05-13 DOI: 10.5194/se-15-589-2024
Matthew S. Hodge, Guri Venvik, Jochen Knies, Roelant van der Lelij, Jasmin Schönenberger, Øystein Nordgulen, Marco Brönner, Aziz Nasuti, Giulio Viola
Abstract. Smøla island, situated within the mid-Norwegian passive margin, contains crystalline-basement-hosted intricate fracture and fault arrays formed during a polyphase brittle tectonic evolution. Its detailed study may strengthen correlation attempts between the well-exposed onshore domain and the inaccessible offshore domain, further the understanding of the passive margin evolution, and provide useful constraints on petrophysical properties of fractured basement blocks. A combination of geophysical and remote sensing lineament analysis, field mapping, high-resolution drill hole logging, 3D modelling, petrographic and microstructural studies, and fault gouge K–Ar geochronology made it possible to define five deformation episodes (D1 to D5). These episodes occurred between the post-Caledonian evolution of the regional-scale Møre–Trøndelag Fault Complex (MTFC) and the Late Cretaceous and younger crustal extension preceding the final stages of Greenland–Norway break-up. Each reconstructed deformation stage is associated with different structural features, fault and fracture geometries, and kinematic patterns. Synkinematic mineralisations evolved progressively from epidote–prehnite, sericite–chlorite–calcite, chlorite–hematite, hematite–zeolite–calcite, to quartz–calcite. K–Ar geochronology constrains brittle deformation to discrete localisation events spanning from the Carboniferous to the Late Cretaceous. Multiscalar geometrical modelling at scales of 100, 10, and 1 m helps constrain the extent and size of the deformation zones of each deformation episode, with D2 structures exhibiting the greatest strike continuity and D1 features the most localised. Overall, the approach highlighted here is of great utility for unravelling complex brittle tectonic histories within basement volumes. It is also a prerequisite to constrain the dynamic evolution of the petrophysical properties of basement blocks.
摘要斯莫拉岛位于挪威被动边缘中部,包含在多相脆性构造演化过程中形成的晶体基性复杂断裂和断层阵列。对该岛的详细研究可能会加强陆上暴露较好的区域与近海难以接近的区域之间的相关性,进一步加深对被动边缘演化的理解,并为断裂基底区块的岩石物理特性提供有用的约束条件。结合地球物理和遥感线型分析、实地测绘、高分辨率钻孔测井、三维建模、岩石学和微结构研究以及断层沟槽 K-Ar 地质年代学,可以确定五个变形期(D1 至 D5)。这些事件发生在区域规模的默勒-特伦德拉格断层群(MTFC)的后卡利登时期演化与格陵兰-挪威断裂最后阶段之前的晚白垩世及更年轻的地壳延伸之间。每个重建的变形阶段都与不同的结构特征、断层和断裂几何形状以及运动模式有关。同步成矿作用从闪锌矿、绢云母-绿泥石-方解石、绿泥石-赤铁矿、赤铁矿-沸石-方解石到石英-方解石逐步演化。K-Ar地质年代学将脆性变形限制在从石炭纪到白垩纪晚期的离散局部事件中。以 100 米、10 米和 1 米的尺度进行的多尺度几何建模有助于确定每个变形事件的变形带的范围和大小,其中 D2 结构表现出最大的走向连续性,而 D1 特征则最具局部性。总之,这里强调的方法对于揭示基底体积内复杂的脆性构造历史非常有用。它也是制约基底岩块岩石物理特性动态演变的先决条件。
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引用次数: 0
Geophysical downhole logging analysis within the shallow depth ICDP STAR drilling project (Central Italy) ICDP STAR 钻探项目(意大利中部)浅层井下地球物理测井分析
IF 3.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-05-13 DOI: 10.5194/egusphere-2024-1249
Paola Montone, Simona Pierdominici, Maria Teresa Mariucci, Francesco Mirabella, Marco Urbani, Assel Akimbekova, Lauro Chiaraluce, Wade Johnson, Massimiliano Rinaldo Barchi
Abstract. The ICDP STAR drilling project aims to study the seismic and aseismic fault slip behaviour of the active low-angle Alto Tiberina normal Fault (ATF) in the Northern Apennines, Central Italy, drilling and instrumenting six shallow boreholes with seismometers and strainmeters. During the STAR field work, a geophysical downhole logging campaign was carried on defining the optimal target depth for instrument deployment and formation rock characterization. In particular, the main objectives of this study were to define in situ physical properties of the rocks and the tectonic discontinuity geometry along the boreholes. The downhole logging data provide new findings and knowledge especially with regards to the physical properties such as resistivity, gamma ray and wave velocity. The collected parameters were compared to the results of literature data collected in similar lithologies, as well as with the results of logging performed in deeper wells drilled for commercial purposes. The physical properties of the Mesozoic-Early Tertiary calcareous formations show low Gamma Ray values and high compressional (Vp) and shear wave (Vs) velocities (up to 5.3 km/s and 2.9 km/s, respectively), whereas the overlying clay-rich Late Tertiary formations exhibit high Gamma Ray and low resistivity and relatively low Vp and Vs values (up to 3.5 km/s and 2.0 km/s, respectively). The results obtained from the analysis of the orientations of the tectonic structures, measured along the six boreholes, show a good agreement with the orientations of the present-day extensional stress field, NE-SW oriented. Our study allowed to bridge the gap between the physical properties obtained from literature data and those obtained from the deep wells measurements, representing a possible case history for future projects. These new data will contribute to the advancement of knowledge of the physical properties of the rocks at shallow depths, typically overlooked.
摘要ICDP STAR 钻探项目旨在研究意大利中部亚平宁半岛北部活跃的低角度 Alto Tiberina 正断层(ATF)的地震和非地震断层滑动行为,该项目使用地震仪和应变仪钻探了六个浅孔并安装了仪器。在 STAR 实地工作期间,进行了一次地球物理井下测井活动,以确定仪器部署和地层岩石特征描述的最佳目标深度。特别是,这项研究的主要目标是确定岩石的现场物理特性和沿钻孔的构造不连续几何形状。井下测井数据提供了新的发现和知识,特别是在电阻率、伽马射线和波速等物理特性方面。收集到的参数与在类似岩性中收集到的文献数据结果以及为商业目的钻探的深井测井结果进行了比较。中生代-早第三纪钙质地层的物理性质显示出较低的伽马射线值以及较高的压缩波(Vp)和剪切波(Vs)速度(分别高达 5.3 千米/秒和 2.9 千米/秒),而上覆富含粘土的晚第三纪地层则显示出较高的伽马射线值和较低的电阻率以及相对较低的 Vp 值和 Vs 值(分别高达 3.5 千米/秒和 2.0 千米/秒)。沿六个钻孔测量的构造结构方向分析结果显示,与当今东北-西南走向的伸展应力场方向十分吻合。我们的研究弥补了从文献数据中获得的物理性质与深井测量获得的物理性质之间的差距,为未来的项目提供了可能的案例。这些新数据将有助于增进人们对通常被忽视的浅层岩石物理性质的了解。
{"title":"Geophysical downhole logging analysis within the shallow depth ICDP STAR drilling project (Central Italy)","authors":"Paola Montone, Simona Pierdominici, Maria Teresa Mariucci, Francesco Mirabella, Marco Urbani, Assel Akimbekova, Lauro Chiaraluce, Wade Johnson, Massimiliano Rinaldo Barchi","doi":"10.5194/egusphere-2024-1249","DOIUrl":"https://doi.org/10.5194/egusphere-2024-1249","url":null,"abstract":"<strong>Abstract.</strong> The ICDP STAR drilling project aims to study the seismic and aseismic fault slip behaviour of the active low-angle Alto Tiberina normal Fault (ATF) in the Northern Apennines, Central Italy, drilling and instrumenting six shallow boreholes with seismometers and strainmeters. During the STAR field work, a geophysical downhole logging campaign was carried on defining the optimal target depth for instrument deployment and formation rock characterization. In particular, the main objectives of this study were to define in situ physical properties of the rocks and the tectonic discontinuity geometry along the boreholes. The downhole logging data provide new findings and knowledge especially with regards to the physical properties such as resistivity, gamma ray and wave velocity. The collected parameters were compared to the results of literature data collected in similar lithologies, as well as with the results of logging performed in deeper wells drilled for commercial purposes. The physical properties of the Mesozoic-Early Tertiary calcareous formations show low Gamma Ray values and high compressional (Vp) and shear wave (Vs) velocities (up to 5.3 km/s and 2.9 km/s, respectively), whereas the overlying clay-rich Late Tertiary formations exhibit high Gamma Ray and low resistivity and relatively low Vp and Vs values (up to 3.5 km/s and 2.0 km/s, respectively). The results obtained from the analysis of the orientations of the tectonic structures, measured along the six boreholes, show a good agreement with the orientations of the present-day extensional stress field, NE-SW oriented. Our study allowed to bridge the gap between the physical properties obtained from literature data and those obtained from the deep wells measurements, representing a possible case history for future projects. These new data will contribute to the advancement of knowledge of the physical properties of the rocks at shallow depths, typically overlooked.","PeriodicalId":21912,"journal":{"name":"Solid Earth","volume":"121 1","pages":""},"PeriodicalIF":3.4,"publicationDate":"2024-05-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140939589","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Driven magmatism and crustal thinning of coastal South China in response to subduction 华南沿海受俯冲作用驱动的岩浆活动和地壳减薄
IF 3.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-05-13 DOI: 10.5194/egusphere-2024-1264
Jinbao Su, Wenbin Zhu, Guangwei Li
Abstract. The late Mesozoic igneous rocks along the coastal South China Block (SCB) exhibit complex parental sources involving a depleted mantle, subducted sediment-derived melt, and melted crust. This period aligns with the magmatic flareup and lull in the SCB, debating with the compression or extension in coastal region. Our study employs numerical models to investigate the dynamics of the ascent of underplating magma along the Changle-Nan’ao Belt (CNB), simulating its intrusion and cooling processes while disregarding the formational background. The rheological structure of the lithospheric mantle significantly influences magma pathways, dictating the distribution of magmatism. This work reveals that the ascent of magma in the presence of faults is considerably faster than that in the absence of faults, and contemporaneous magmatic melts could produce different cooling and diagenetic processes. Additionally, the influence of pre-existing magma accelerates underplating magma emplacement. The ascending of magma forms a mush-like head, contributing to magmatic circulation beneath the crust and decreasing crustal thickness. Multiphase magmatism increases the geothermal gradient, reducing the lithospheric viscosity and promoting underplating magma ascent, leading to magmatic flare-ups and lulls. Our findings suggest that the Cretaceous magmatism at different times in the coastal SCB may be associated with the effects of lithospheric faults under similar subduction conditions. Boundary compression forces delay magma ascent, while rising magma induces a significant circulation, decreasing the crustal thickness of the coastal SCB. This study provides new insights into the complex interplay of magmatic processes during subduction, emphasizing the role of lithospheric structure in shaping the temporal and spatial evolution of coastal magmatism.
摘要华南地块沿岸中生代晚期火成岩表现出复杂的成因,包括贫化的地幔、俯冲沉积物衍生的熔体和熔融的地壳。这一时期与华南地块的岩浆爆发和沉寂相一致,与沿岸地区的压缩或延伸存在争论。我们的研究采用数值模式研究了长乐-南澳带的下伏岩浆上升动力学,模拟了岩浆的侵入和冷却过程,同时忽略了形成背景。岩石圈地幔的流变结构对岩浆路径有重大影响,决定了岩浆活动的分布。这项工作揭示了存在断层的岩浆上升速度大大快于不存在断层的岩浆上升速度,同时代的岩浆熔体可能产生不同的冷却和成岩过程。此外,先期存在的岩浆的影响加速了板下岩浆的喷发。岩浆的上升会形成一个蘑菇状的岩浆头,促进地壳下的岩浆循环,减小地壳厚度。多相岩浆活动增加了地热梯度,降低了岩石圈的粘度,促进了欠增生岩浆的上升,导致岩浆爆发和岩浆沉积。我们的研究结果表明,南中北沿海不同时期的白垩纪岩浆活动可能与类似俯冲条件下岩石圈断层的影响有关。边界压缩力延迟了岩浆的上升,而上升的岩浆引起了显著的环流,减小了沿岸华南板块的地壳厚度。这项研究为了解俯冲过程中岩浆过程的复杂相互作用提供了新的视角,强调了岩石圈结构在塑造沿岸岩浆活动的时空演变过程中的作用。
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引用次数: 0
The influence of viscous slab rheology on numerical models of subduction 粘性板块流变学对俯冲数值模型的影响
IF 3.4 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-05-07 DOI: 10.5194/se-15-567-2024
Natalie Hummel, Susanne Buiter, Zoltán Erdős
Abstract. Numerical models of subduction commonly use diffusion and dislocation creep laws from laboratory deformation experiments to determine the rheology of the lithosphere. The specific implementation of these laws varies from study to study, and the impacts of this variation on model behavior have not been thoroughly explored. We run simplified 2D numerical models of free subduction in SULEC, with viscoplastic slabs following (1) a diffusion creep law, (2) a dislocation creep law, and (3) both simultaneously, as well as several variations of model 3 with reduced resistance to bending. We compare the results of these models to a model with a constant-viscosity slab to determine the impact of the implementation of different lithospheric flow laws on subduction dynamics. In creep-governed models, higher subduction velocity causes a longer effective slab length, increasing slab pull and asthenospheric drag, which, in turn, affect subduction velocity. Numerical and analogue models implementing constant-viscosity slabs lack this feedback but still capture morphological patterns observed in more complex models. Dislocation creep is the primary deformation mechanism throughout the subducting lithosphere in our models. However, both diffusion creep and dislocation creep predict very high viscosities in the cold core of the slab. At the trench, the effective viscosity is lowered by plastic failure, rendering effective slab thickness the primary control on bending resistance and subduction velocity. However, at depth, plastic failure is not active, and the viscosity cap is reached in significant portions of the slab. The resulting high slab stiffness causes the subducting plate to curl under itself at the mantle transition zone, affecting patterns in subduction velocity, slab dip, and trench migration over time. Peierls creep and localized grain size reduction likely limit the stress and viscosity in the cores of real slabs. Numerical models implementing only power-law creep and neglecting Peierls creep are likely to overestimate the stiffness of subducting lithosphere, which may impact model results in a variety of respects.
摘要。俯冲的数值模型通常使用实验室变形实验中的扩散和位错蠕变定律来确定岩石圈的流变学。不同的研究对这些定律的具体实现方法不尽相同,这种变化对模型行为的影响尚未得到深入探讨。我们运行了 SULEC 自由俯冲的简化二维数值模型,粘塑性板块遵循(1)扩散蠕变规律;(2)位错蠕变规律;(3)同时遵循这两种规律;以及模型 3 的几种变体,它们的弯曲阻力都减小了。我们将这些模型的结果与恒定粘度板块模型进行比较,以确定实施不同岩石圈流动规律对俯冲动力学的影响。在蠕变控制的模型中,较高的俯冲速度会导致较长的有效板坯长度,增加板坯拉力和星体层阻力,反过来又影响俯冲速度。实施恒定粘度板坯的数值和模拟模型缺乏这种反馈,但仍能捕捉到在更复杂模型中观察到的形态模式。在我们的模型中,位错蠕变是整个俯冲岩石圈的主要变形机制。然而,无论是扩散蠕变还是位错蠕变,都预示着板块冷核的粘度非常高。在海沟处,塑性破坏降低了有效粘度,使有效板坯厚度成为弯曲阻力和俯冲速度的主要控制因素。然而,在板块深处,塑性破坏并不活跃,板块的很大一部分都达到了粘度上限。由此产生的高板坯刚度导致俯冲板块在地幔过渡带向自身下方弯曲,从而影响俯冲速度、板坯倾角和海沟迁移的模式。Peierls 蠕变和局部粒度减小可能会限制实际板块核心的应力和粘度。只采用幂律蠕变而忽略佩尔蠕变的数值模型很可能会高估俯冲岩石圈的刚度,这可能会对模型结果产生多方面的影响。
{"title":"The influence of viscous slab rheology on numerical models of subduction","authors":"Natalie Hummel, Susanne Buiter, Zoltán Erdős","doi":"10.5194/se-15-567-2024","DOIUrl":"https://doi.org/10.5194/se-15-567-2024","url":null,"abstract":"Abstract. Numerical models of subduction commonly use diffusion and dislocation creep laws from laboratory deformation experiments to determine the rheology of the lithosphere. The specific implementation of these laws varies from study to study, and the impacts of this variation on model behavior have not been thoroughly explored. We run simplified 2D numerical models of free subduction in SULEC, with viscoplastic slabs following (1) a diffusion creep law, (2) a dislocation creep law, and (3) both simultaneously, as well as several variations of model 3 with reduced resistance to bending. We compare the results of these models to a model with a constant-viscosity slab to determine the impact of the implementation of different lithospheric flow laws on subduction dynamics. In creep-governed models, higher subduction velocity causes a longer effective slab length, increasing slab pull and asthenospheric drag, which, in turn, affect subduction velocity. Numerical and analogue models implementing constant-viscosity slabs lack this feedback but still capture morphological patterns observed in more complex models. Dislocation creep is the primary deformation mechanism throughout the subducting lithosphere in our models. However, both diffusion creep and dislocation creep predict very high viscosities in the cold core of the slab. At the trench, the effective viscosity is lowered by plastic failure, rendering effective slab thickness the primary control on bending resistance and subduction velocity. However, at depth, plastic failure is not active, and the viscosity cap is reached in significant portions of the slab. The resulting high slab stiffness causes the subducting plate to curl under itself at the mantle transition zone, affecting patterns in subduction velocity, slab dip, and trench migration over time. Peierls creep and localized grain size reduction likely limit the stress and viscosity in the cores of real slabs. Numerical models implementing only power-law creep and neglecting Peierls creep are likely to overestimate the stiffness of subducting lithosphere, which may impact model results in a variety of respects.","PeriodicalId":21912,"journal":{"name":"Solid Earth","volume":"23 1","pages":""},"PeriodicalIF":3.4,"publicationDate":"2024-05-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140887666","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
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