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Formation of high-silica adakites and their relationship with slab break-off: Implications for generating fertile Cu-Au-Mo porphyry systems 高硅方解石的形成及其与板块断裂的关系:对生成肥沃的铜-金-钼斑岩系统的影响
IF 8.5 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-09-10 DOI: 10.1016/j.gsf.2024.101927
Fazilat Yousefi, David R. Lentz
<div><p>In recent years, the characteristics and sources of fertile adakites has received considerable attention. As well, most recently the geodynamic environment of convergent margins subducting oceanic crust aiding arc formation, evolving to slab rollback, then slab break-off after collision (i.e. late- to post-collisional slab failure (arc-like magmatism) and transpression) has gained more recognition, although their relationship to each other has yet to be explored. The geochemical characteristics imply that adakites/adakite-like, in particular high-silica adakites (HSA), can form by partial melting of subducting hydrothermally altered oceanic crust in convergent plate boundary settings during the terminal stages of subduction, lithosphere thickening, and then failure (all late to post collisional), while the melting of the mantle wedge during subduction-related dehydration creates more typical calc-alkaline basalt-andesite-dacite-rhyolite series (ADR) to form intraoceanic island arc to intracontinental margin arc systems, before the collisional stage. HSAs are characterized by high-silica (SiO<sub>2</sub> > 67 wt.%), Al<sub>2</sub>O<sub>3</sub> > 15 wt.%, Sr > 300 ppm, Y<20 ppm, Yb < 1.8 ppm, and Nb ≤ 10 ppm, and MgO < 3 wt.%, with high Sr/Y (>50), and La/Yb (>10). Some specific geochemical features, such as high Mg# (ave 0.51), Ni (ave 924 ppm), and Cr (ave 36 ppm), in HSAs are typical, in contrast to calc-alkaline arcs, although both groups display similar but less pronounced negative anomalies of Nb, Ta, and Ti in primitive mantle-normalized trace element spider diagram profiles. These unique geochemical features are likely ascribed to the involvement of garnet, hornblende, and titanite either during partial melting of hydrous MORB-like oceanic crust with only minor assimilation and fractional crystallization (AFC) within the mantle and crustal during ascent in a transpressional collisional environment. Hypotheses for origin of HSA derivative from melting in convergent margins from young, hot oceanic plates subducting into the mantle is applicable to only some adakitic systems. The difference in geochemical characteristics of adakites compared to ADR, such as relative higher MgO, Cr, Cu, and Ni, are due to their slab source, as well as interaction of the slab-derived adakitic melts with overlying hot lithospheric mantle; altered oceanic slabs are also relatively rich in siderophile and other chalcophile elements, as well as sulfates and sulfides. HSA magmas related to slab failure have special geochemical properties, such as Sr/Y > 20, Nb/Y > 0.4, Ta/Yb > 0.3, La/Yb > 10, Gd/Yb > 2, and Sm/Yb > 2.5. Slightly higher Nb + Ta is due to high <em>T</em> melting of rutile. Varieties of Nb/Ta compared to silica are also significant in HSA as a result of slab failure (roll back to break-off). High <em>T</em>-<em>P</em> partial melting of the hydrothermally altered oceanic slab produces HSA with quite hig
近年来,肥沃阿达克岩的特征和来源受到了广泛关注。最近,汇聚边俯冲大洋地壳帮助弧的形成、演变为板块后退、碰撞后板块断裂(即碰撞后期至碰撞后板块破坏(弧状岩浆活动)和转位)的地球动力环境也得到了更多的认可,尽管它们之间的关系还有待探讨。地球化学特征表明,在俯冲、岩石圈增厚的末期阶段,在板块交汇边界环境中,俯冲热液蚀变的大洋地壳部分熔化后,可形成吸积岩/类吸积岩,特别是高硅吸积岩(HSA)、而地幔楔在与俯冲有关的脱水过程中的熔化则形成了更典型的钙碱性玄武岩-安山岩-黑云母-流纹岩系列(ADR),从而在碰撞阶段之前形成洋内岛弧至洲内边缘弧系统。HSA的特征是高硅(SiO2 67%)、Al2O3 15%、Sr 300ppm、Y 20ppm、Yb 1.8ppm、Nb ≤ 10ppm、MgO 3%,以及高Sr/Y(50)和La/Yb(10)。一些特殊的地球化学特征,如高 Mg#(平均值 0.51)、Ni(平均值 924 ppm)和 Cr(平均值 36 ppm),在 HSAs 中是典型的,与钙碱性弧形成鲜明对比,尽管这两类弧在原始地幔归一化微量元素蛛网图剖面中显示出类似但不太明显的 Nb、Ta 和 Ti 负异常。这些独特的地球化学特征很可能是由于石榴石、角闪石和榍石的参与,或者是在类水MORB洋壳部分熔融过程中的参与,或者是在换位碰撞环境中上升过程中地幔和地壳内仅有少量同化和部分结晶(AFC)的参与。关于HSA衍生物起源于年轻、炽热的大洋板块向地幔俯冲的汇聚边缘熔融的假设,只适用于某些阿达克特系统。与 ADR 相比,adakites 的地球化学特征有所不同,如相对较高的氧化镁、铬、铜和镍,这是由于它们的板块来源,以及板块衍生的 adakitic 熔体与上覆热岩石圈地幔的相互作用造成的;蚀变的大洋板块也相对富含亲凫元素和其他亲铬元素,以及硫酸盐和硫化物。与板块崩塌有关的 HSA 岩浆具有特殊的地球化学性质,如 Sr/Y >20、Nb/Y >0.4、Ta/Yb >0.3、La/Yb >10、Gd/Yb >2、Sm/Yb >2.5。Nb + Ta 略高是因为金红石的高 T 熔化。与二氧化硅相比,Nb/Ta 的变化在 HSA 中也很明显,这是板坯破坏(回滚到断裂)的结果。热液蚀变的大洋板块的高T-P部分熔化产生了HSA,其中H2O、SO2、HCl的活度相当高,而亲铝金属在较高的fO2(低fH2)条件下仍然不相容;这种情况发生在碰撞晚期至碰撞后的环境中,在这种环境中,俯冲的大洋地壳经历了板块崩塌,导致上涌的岩石圈向系统增加平流热量。在这种板块破裂的情况下,转位和横张在大量肥沃的阿达基岩浆通过俯冲改造的岩石圈和地壳快速置入上地壳中起着重要作用。当氧化板块熔体与俯冲改造岩石圈地幔相互作用时,产生的岩浆保持氧化状态,有可能促成有利于形成斑岩型铜金矿化的特殊条件。
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引用次数: 0
Tectonic controls on ore deposit exhumation and preservation: A case study of the Handan-Xingtai iron-skarn district 构造对矿床出露和保存的控制:邯郸-邢台铁矽卡岩区案例研究
IF 8.5 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-09-10 DOI: 10.1016/j.gsf.2024.101924
Yannan Wang , Zhiyuan He , Kai Bian , Cunliang Zhao , Lian Chen , Rui Dong , Jin Zhang , Zhaoqun Zhu , Guang Liu

Despite the growing concern regarding post-mineralization thermo-tectonic processes in recent years, the relative roles in exhuming and preserving ore deposits remain highly controversial. This study presents new apatite fission track and (U-Th)/He data from the Xishimen iron skarn deposit in the Handan-Xingtai district, central North China Craton. Apatite fission track dating yielded central ages ranging from 88 ± 18 Ma to 125 ± 9 Ma, with mean confined track lengths varying between 11.9 ± 0.4 μm and 13.3 ± 0.2 μm. Integrated apatite (U-Th)/He dating provided ages of 42.5 ± 0.8 Ma to 48.1 ± 3.3 Ma. Our new data, combined with previous zircon U-Pb and potassium-bearing mineral 40Ar/39Ar ages, revealed three cooling episodes: very rapid cooling (100–140 °C/Ma) at ca. 130–120 Ma, a protracted slow cooling period (0.2–0.4 °C/Ma) at ca. 120–50 Ma, and moderate cooling (0.8–1.0 °C/Ma) since ca. 50 Ma. The initial rapid cooling phase was primarily attributed to post-magmatic thermal equilibration following the shallow emplacement of the Xishimen deposit. The subsequent cooling phases were controlled by uplift and exhumation processes. Our thermal models indicate an estimated total unroofing thickness of < 3 km, which is shallower than the emplacement depth of the ore deposit (3–5 km). This suggests significant potential for mineral exploration. Furthermore, a comprehensive review of preservation mechanisms for various ore deposits underscores the significant role of tectonics in both exhuming and preserving ore bodies.

尽管近年来人们越来越关注成矿后的热构造过程,但对矿床出露和保存的相对作用仍存在很大争议。本研究提供了华北克拉通中部邯郸-邢台地区西石门铁矽卡岩矿床新的磷灰石裂变轨迹和(U-Th)/He数据。磷灰石裂变轨迹测年得出的中心年龄为88±18Ma至125±9Ma,平均封闭轨迹长度为11.9±0.4μm至13.3±0.2μm。磷灰石(U-Th)/He综合测年提供了 42.5 ± 0.8 Ma 至 48.1 ± 3.3 Ma 的年龄。我们的新数据与之前的锆石 U-Pb 和含钾矿物 40Ar/39Ar 年龄相结合,揭示了三个冷却过程:约 130-120 Ma 时的极速冷却(100-140 °C/Ma)、约 130-120 Ma 时的长期冷却(100-140 °C/Ma)、约 130-120 Ma 时的长期冷却(100-140 °C/Ma)。约 130-120 Ma 时的极快速冷却(100-140 °C/Ma),约 120-50 Ma 时的长期缓慢冷却(0.2-0.4 °C/Ma),以及中度冷却(0.2-0.4 °C/Ma)。120-50Ma,以及自约 50Ma 开始的中度冷却(0.8-1.0 °C/Ma)。从大约 50 Ma 开始的中度冷却(0.8-1.0 °C/Ma)。最初的快速冷却阶段主要归因于西石门沉积层浅部置入后的岩浆热平衡。随后的冷却阶段则由隆起和掘起过程控制。我们的热模型表明,估计的总揭露厚度为 3 千米,比矿床的堆积深度(3-5 千米)要浅。这表明这里具有巨大的矿产勘探潜力。此外,对各种矿床保存机制的全面审查强调了构造作用在矿体出露和保存方面的重要作用。
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引用次数: 0
Spatio-temporal analysis of Permian-Cretaceous magmatic activities in the Tengchong block: Implications for tectono-magmatic evolution 腾冲地块二叠纪-白垩纪岩浆活动的时空分析:构造岩浆演化的意义
IF 8.5 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-08-31 DOI: 10.1016/j.gsf.2024.101920
Xinkun Yang , Zhenjie Zhang , Yuanzhi Zhou , Jie Yang

Understanding the tectono-magmatic evolution history of the Tengchong block is crucial for elucidating the formation of the Eastern Tethys tectonic domain. However, the correlation and evolution of the Tengchong block with the Sibumasu and Lhasa blocks is controversial during the Permian and Cretaceous. This study explores the information contained within magmatic rocks using big data and spatio-temporal analysis, providing quantitative constraints for the discussion of the tectono-magmatic evolution of the Tengchong block. To more accurately assess true magma activities and reduce errors caused by preservation and sampling processes, we utilized local singularity analysis to obtain the singularity index time-series. Correlation analysis of zircon ages and εHf(t) (correlation coefficient ≥ 0.5) values indicates that the Tengchong block is more similar to the Sibumasu block. Results from time-lagged cross-correlation analysis indicate that the Tengchong block and Sibumasu block exhibit a shorter lag in magmatic activities (3 Myr). Wavelet analysis reveals similar periods of collision-related magmatic activities (57 Myr and 43 Myr). Integrating evidence from paleontology and ophiolite belts, we propose that the Tengchong block co-evolved more closely with the Sibumasu block than with the Lhasa block, suggesting similar tectonic processes during the Early Permian to Early Cretaceous. Approximately 250–236 Ma, in the western Tengchong block, partial melting of the lower crust occurs due to crustal thickening. Around 219–213 Ma and 198–180 Ma, after the Tengchong block collided with the Eurasian continent, the subduction of the Meso-Tethys Ocean commenced. Around 130–111 Ma, the overall tectonic feature was a scissor-like closure of the Meso-Tethys Ocean from north to south.

了解腾冲块体的构造-岩浆演化史对于阐明东特提斯构造域的形成至关重要。然而,在二叠纪和白垩纪,腾冲地块与西双版纳和拉萨地块的相关性和演化却存在争议。本研究利用大数据和时空分析,探索岩浆岩所蕴含的信息,为探讨腾冲块体的构造-岩浆演化提供定量约束。为了更准确地评估岩浆活动的真实情况,减少保存和取样过程造成的误差,我们利用局部奇异性分析获得了奇异性指数时间序列。锆石年龄与εHf(t)(相关系数≥0.5)值的相关分析表明,腾冲块体与西布玛苏块体更为相似。时滞交叉相关分析结果表明,腾冲块体和西布玛苏块体的岩浆活动滞后时间较短(3 Myr)。小波分析显示,与碰撞有关的岩浆活动期相似(57 Myr 和 43 Myr)。综合古生物学和蛇绿岩带的证据,我们认为腾冲块体与西双版纳块体的共同演化比与拉萨块体的共同演化更为密切,这表明早二叠世至早白垩世的构造过程相似。大约在250-236Ma,腾冲西部地块由于地壳增厚,下地壳发生部分融化。约 219-213 Ma 和 198-180 Ma,腾冲地块与欧亚大陆碰撞后,中特提斯洋开始俯冲。在 130-111 Ma 前后,中特提斯洋的总体构造特征是自北向南呈剪刀状闭合。
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引用次数: 0
Evaluation of gas content in organic-rich shale: A review of the history, current status, and future directions 富含有机质页岩中气体含量的评估:历史、现状和未来方向回顾
IF 8.5 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-08-31 DOI: 10.1016/j.gsf.2024.101921
Haikuan Nie , Wei Dang , Qin Zhang , Jinchuan Zhang , Pei Li , Shaohua Zhang , Jianghui Ding , Qian Chen , Yubo Feng , Xin Zhang

Shale gas is being hailed as the green energy of the future due to high heating value, low carbon emissions, and large reserves. Gas content of shale is a key parameter for evaluating the shale gas potential and screening for the shale gas sweet spots. Although the concept of gas content has been well defined, obtaining a reliable gas content data still remains a challenge. A significant barrier is the method for evaluating the gas content. In this paper, we provide a review of the long-established and recently developed gas content evaluation methods. In the first part of this review article, the history of gas content evaluation methods is summarized since 1910s, relied on published and unpublished literatures as well as our own experiences. Then, the fundamental contents and concepts involved in gas content evaluation are introduced to provide a clear theoretical foundation for the methods. In the third part, eleven evaluation methods, including four direct methods and seven indirect methods, are systematically reviewed. In each method, its application to evaluating the gas content is presented, the key advances are highlighted, and the advantages and limitations are discussed. Finally, future directions are discussed to promote creative thinking across disciplines to develop new methods or improve current methods for evaluating the gas content more accurately and efficiently.

页岩气因热值高、碳排放量低、储量大而被誉为未来的绿色能源。页岩的含气量是评估页岩气潜力和筛选页岩气甜点的关键参数。虽然含气量的概念已经得到了很好的定义,但获取可靠的含气量数据仍然是一项挑战。一个重要的障碍就是含气量的评估方法。在本文中,我们将对历史悠久和最新开发的含气量评估方法进行综述。在综述文章的第一部分,我们根据已发表和未发表的文献以及自身的经验,总结了自 1910 年代以来气体含量评估方法的历史。然后,介绍了气体含量评价所涉及的基本内容和概念,为这些方法提供了清晰的理论基础。第三部分系统回顾了 11 种评价方法,包括 4 种直接方法和 7 种间接方法。每种方法都介绍了其在含气量评价中的应用,强调了主要进展,并讨论了其优势和局限性。最后,讨论了未来的发展方向,以促进跨学科的创造性思维,开发新方法或改进现有方法,从而更准确、更高效地评估气体含量。
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引用次数: 0
Earth’s tectonic and plate boundary evolution over 1.8 billion years 18 亿年来地球构造和板块边界的演变
IF 8.5 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-08-31 DOI: 10.1016/j.gsf.2024.101922
Xianzhi Cao , Alan S. Collins , Sergei Pisarevsky , Nicolas Flament , Sanzhong Li , Derrick Hasterok , R. Dietmar Müller

Understanding the intricate relationships between the solid Earth and its surface systems in deep time necessitates comprehensive full-plate tectonic reconstructions that include evolving plate boundaries and oceanic plates. In particular, a tectonic reconstruction that spans multiple supercontinent cycles is important to understand the long-term evolution of Earth’s interior, surface environments and mineral resources. Here, we present a new full-plate tectonic reconstruction from 1.8 Ga to present that combines and refines three published models: one full-plate tectonic model spanning 1 Ga to present and two continental-drift models focused on the late Paleoproterozoic to Mesoproterozoic eras. Our model is constrained by geological and geophysical data, and presented as a relative plate motion model in a paleomagnetic reference frame. The model encompasses three supercontinents, Nuna (Columbia), Rodinia, and Gondwana/Pangea, and more than two complete supercontinent cycles, covering ∼40% of the Earth’s history. Our refinements to the base models are focused on times before 1.0 Ga, with minor changes for the Neoproterozoic. For times between 1.8 Ga and 1.0 Ga, the root mean square speeds for all plates generally range between 4 cm/yr and 7 cm/yr (despite short-term fast motion around 1.1 Ga), which are kinematically consistent with post-Pangean plate tectonic constraints. The time span of the existence of Nuna is updated to between 1.6 Ga (1.65 Ga in the base model) and 1.46 Ga based on geological and paleomagnetic data. We follow the base models to leave Amazonia/West Africa separate from Nuna (as well as Western Australia, which only collides with the remnants of Nuna after initial break-up), and South China/India separate from Rodinia. Contrary to the concept of a “boring billion”, our model reveals a dynamic geological history between 1.8 Ga and 0.8 Ga, characterized by supercontinent assembly and breakup, and continuous accretion events. The model is publicly accessible, providing a framework for future refinements and facilitating deep time studies of Earth’s system. We suggest that the model can serve as a valuable working hypothesis, laying the groundwork for future hypothesis testing.

要了解固体地球及其表面系统在深部时间的复杂关系,就必须进行全面的全板块构造重建,其中包括不断演变的板块边界和大洋板块。特别是,跨越多个超大陆周期的构造重建对于了解地球内部、地表环境和矿产资源的长期演化非常重要。在这里,我们提出了一个从 1.8 Ga 到现在的新的全板块构造重建,它结合并完善了三个已发表的模型:一个跨越 1 Ga 到现在的全板块构造模型和两个侧重于晚古生代到中古生代的大陆漂移模型。我们的模型受到地质和地球物理数据的制约,是在古地磁参考框架下的相对板块运动模型。该模型包括三个超大陆,即努纳大陆(哥伦比亚)、罗迪尼亚大陆和冈瓦纳/泛大陆,以及两个以上完整的超大陆周期,涵盖了地球历史的 40%。我们对基本模型的改进主要集中在 1.0 Ga 之前,对新近纪略有改动。在 1.8 Ga 到 1.0 Ga 之间,所有板块的均方根速度一般在 4 cm/yr 到 7 cm/yr 之间(尽管在 1.1 Ga 附近有短期的快速运动),这在运动学上与后泛大陆板块构造的约束相一致。根据地质和古地磁数据,努纳存在的时间跨度更新为 1.6 Ga(基础模型为 1.65 Ga)和 1.46 Ga 之间。我们沿用了基础模型,将亚马孙/西非从努纳星分离出来(以及西澳大利亚,它只是在最初解体后才与努纳星的残余部分相撞),并将华南/印度从罗迪尼亚分离出来。与 "无聊的十亿 "概念相反,我们的模型揭示了 1.8 Ga 到 0.8 Ga 之间的动态地质历史,其特点是超大陆的组装和解体,以及持续的增生事件。该模型可公开访问,为未来的改进提供了一个框架,并促进了对地球系统的深时研究。我们认为该模型可以作为一个有价值的工作假设,为未来的假设检验奠定基础。
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引用次数: 0
Multifaceted natural resources and green energy transformation for sustainable industrial development 多元自然资源和绿色能源转型促进可持续工业发展
IF 8.5 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-08-24 DOI: 10.1016/j.gsf.2024.101919
Desire Wade Atchike , Munir Ahmad , Qingyu Zhang

Climate change is the most phenomenal challenge to humanity, and its roots are intervened with unsustainable industrialization, exercising overexploitation of natural resources. Therefore, the departure from non-renewable to renewables has become inevitable, though thought-provoking. In this respect, we explore how green energy transformation moderates the impacts of multifaceted natural resources on sustainable industrial development in the presence of other covariates involving technological progress, financial development, and economic progress. We compiled data from Group of Seven (G-7) members over the 1995−2018 period and applied panel quantile regression (PQREG) to capture the effects across varying levels of quantiles of sustainable industrial development. Results revealed a positive role of natural gas rents, while coal, forest, and total natural resource rents contributed adverse implications for sustainable industrial development. However, the green energy transformation proved to be the game changer because it not only directly induced sustainable industrial development improvement but also turned the unfavorable effects of coal, forest, and total natural resources into favorable ones by interacting with those multifaceted natural resources. Technological, financial, and economic progress supported sustainable industrial development in G-7 nations, particularly in members with existing middle and upper scales of sustainable industrial development. These findings are robust enough when subjected to different estimation tools. In light of these outcomes, the interaction between green energy transformation and natural resource policy is inevitably critical to attaining natural resource efficiency for sustainable industrial development. Therefore, it is imperative to establish a close policy coordination between advancing green energy technology and allocating natural resource revenue to achieve sustainable development goals (SDGs), with a particular emphasis on SDG-7 and SDG-13.

气候变化是人类面临的最大挑战,其根源在于不可持续的工业化和对自然资源的过度开发。因此,从不可再生能源到可再生能源的转变已成为不可避免的趋势,尽管这一转变发人深省。为此,我们探讨了在技术进步、金融发展和经济进步等其他协变量存在的情况下,绿色能源转型如何调节多元自然资源对工业可持续发展的影响。我们汇编了七国集团(G-7)成员国 1995-2018 年期间的数据,并应用面板量化回归(PQREG)来捕捉不同量化水平的可持续工业发展的影响。结果显示,天然气租金发挥了积极作用,而煤炭、森林和自然资源总租金则对工业可持续发展产生了不利影响。然而,事实证明绿色能源转型改变了游戏规则,因为它不仅直接促使工业可持续发展得到改善,而且通过与煤炭、森林和自然资源总量等多方面的相互作用,将这些不利影响转化为有利影响。技术、金融和经济进步支持了七国集团国家的可持续工业发展,尤其是在可持续工业发展水平处于中上游的国家。这些发现在使用不同的估算工具时都非常可靠。鉴于这些结果,绿色能源转型与自然资源政策之间的互动对于实现自然资源效率以促进可持续工业发展必然至关重要。因此,为实现可持续发展目标(SDGs),特别是 SDG-7 和 SDG-13 目标,必须在推进绿色能源技术与自然资源收入分配之间建立密切的政策协调。
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引用次数: 0
A reliability analysis framework coupled with statistical uncertainty characterization for geotechnical engineering 可靠性分析框架与岩土工程统计不确定性表征相结合
IF 8.5 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-08-22 DOI: 10.1016/j.gsf.2024.101913
Liang Han , Wengang Zhang , Lin Wang , Jia Fu , Liang Xu , Yu Wang

Reliability analysis plays an important role in the risk management of geotechnical engineering. For the random field-based method, it is expected that the uncertainty characterization of geo-material parameters and the realization of random field can be integrated effectively. Moreover, as the increase in measured data size is generally difficult in the field investigation of geotechnical engineering due to limitation of budget and time etc., the statistical uncertainty resulting from sparse data should be paid great attention. Therefore, taking the determination of hyper-parameters for Bayesian-based conditional random field as the breakthrough, this study proposed a reliability analysis framework to achieve the expectation above. In this proposed reliability analysis framework, the present characterization method of statistical uncertainty is improved by setting the lognormal distribution as the prior distribution of scale of fluctuation (SOF). Subsequently, the performance of statistical uncertainty characterization method is tested by a set of unconfined compressive strength (UCS) database about rocks. Then, a case study about the stability analysis of slope is employed to demonstrate the beneficial effect of the proposed reliability analysis framework. It is found that the uncertainty in both the realization of random field and the reliability analysis results can be significantly mitigated by the proposed reliability analysis framework.

可靠性分析在岩土工程风险管理中发挥着重要作用。对于基于随机场的方法而言,预计可以将土工材料参数的不确定性表征与随机场的实现有效地结合起来。此外,在岩土工程现场勘察中,由于受到预算和时间等因素的限制,一般很难增加实测数据量,因此应高度重视数据稀疏导致的统计不确定性。因此,本研究以基于贝叶斯的条件随机场超参数的确定为突破口,提出了一种可靠性分析框架来实现上述预期。在本研究提出的可靠性分析框架中,通过将对数正态分布设为波动标度(SOF)的先验分布,改进了现有的统计不确定性表征方法。随后,通过一组有关岩石的非收缩抗压强度(UCS)数据库测试了统计不确定性表征方法的性能。然后,以边坡稳定性分析为案例,展示了所提出的可靠性分析框架的有益效果。研究发现,建议的可靠性分析框架可显著降低随机场实现和可靠性分析结果的不确定性。
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引用次数: 0
Early terrestrial and lunar anorthosites: Comparative geochemistry and evolutionary processes 早期陆地和月球正长岩:比较地球化学和进化过程
IF 8.5 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-08-20 DOI: 10.1016/j.gsf.2024.101914
Paul Sotiriou , Ali Polat , Tim Kusky , Brian F. Windley

In a paper in 1970, Brian Windley first recognised that early terrestrial and lunar anorthosites both have calcic plagioclase, and low TiO2 and high CaO and Al2O3 contents. Despite these similarities, the geochemistry of early terrestrial and lunar anorthosites has not been rigorously compared and contrasted. To this end, we compiled 425 analyses from 212 early terrestrial anorthosite occurrences and 306 analyses from 16 lunar anorthosite occurrences. This was supplemented by a compilation of plagioclase anorthite (An) contents and pyroxene Mg# from early terrestrial and lunar anorthosites. Early terrestrial anorthosites have lower whole-rock An contents but similar Mg# to lunar anorthosites. The CaO contents of lunar anorthosites are higher than those of early terrestrial anorthosites for a given MgO and Al2O3 content, early terrestrial anorthosites have higher SiO2 contents than lunar anorthosites at a given MgO content, and lunar anorthosites have higher Eu/Eu* anomaly ratios yet broadly similar La/Yb and Nd/Sm ratios than early terrestrial anorthosites. Some early terrestrial anorthosites have less fractionated chondrite-normalised rare earth element (REE) patterns and less prominent positive Eu anomalies than lunar anorthosites. Lunar anorthosites have higher plagioclase An contents, yet a similar range of pyroxene Mg# compared to their early terrestrial counterparts. Some early terrestrial anorthosites are more fractionated than some lunar anorthosites. Our interpretations imply that most early terrestrial anorthosites crystallised from basaltic parental magmas that were generated by high-degree partial melting of sub-arc asthenosphere mantle wedge sources that were hydrated by slab-derived fluids, with the remainder being associated with mid-ocean ridge and mantle plume settings. Some of the arc-related early terrestrial anorthosites were influenced by crustal contamination. In addition, early terrestrial anorthosites originated from partial melting of the mantle at various depths with variable garnet residua, whereas lunar anorthosites formed without any significant garnet residua. Lower plagioclase CaO contents and pyroxene Mg# in early terrestrial anorthosites can be explained by higher proportions of clinopyroxene and olivine fractionation in terrestrial magma chambers than in the lunar magma ocean where orthopyroxene and olivine fractionation occurred. Low TiO2 contents in both terrestrial and lunar anorthosites reflect rutile and/or ilmenite fractionation.

布莱恩-温德利(Brian Windley)在 1970 年的一篇论文中首次指出,早期陆地和月球正长岩都具有钙斜长石、低 TiO2 含量、高 CaO 和 Al2O3 含量。尽管存在这些相似之处,但早期陆地和月球正长岩的地球化学还没有进行过严格的比较和对比。为此,我们汇编了 212 个早期陆地正长岩矿点的 425 项分析结果和 16 个月球正长岩矿点的 306 项分析结果。此外,我们还汇编了早期陆地和月球正长岩的斜长石正长石(An)含量和辉石 Mg#。早期陆地正长岩的全岩 An 含量较低,但 Mg# 与月球正长岩相似。在氧化镁和氧化铝含量一定的情况下,月球正长岩的氧化钙含量高于早期陆地正长岩;在氧化镁含量一定的情况下,早期陆地正长岩的二氧化硅含量高于月球正长岩;月球正长岩的Eu/Eu*异常比高于早期陆地正长岩,但La/Yb和Nd/Sm比大致相似。与月球正长岩相比,一些早期陆地正长岩的稀土元素(REE)模式分馏程度较低,正Eu异常也不那么突出。与早期陆地正长岩相比,月球正长岩的斜长石An含量较高,但辉石Mg#的范围相似。与某些月球正长岩相比,某些早期陆地正长岩的分馏程度更高。我们的解释意味着,大多数早期陆地正长岩是由玄武质母岩结晶而成的,这些母岩是由弧下天体层地幔楔源的高度部分熔融产生的,并被板块衍生流体水化,其余的则与洋中脊和地幔羽流环境有关。一些与弧有关的早期陆地正长岩受到地壳污染的影响。此外,早期陆地正长岩源于地幔在不同深度的部分熔化,其石榴石残留物各不相同,而月球正长岩的形成则没有任何明显的石榴石残留物。早期陆地正长岩中斜长石 CaO 含量和辉石 Mg# 含量较低的原因是陆地岩浆室中的挛辉石和橄榄石分馏比例高于月球岩浆洋中的正长石和橄榄石分馏比例。陆相和月相正长岩中较低的二氧化钛含量反映了金红石和/或钛铁矿的分馏。
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引用次数: 0
Long-term daily water temperatures unveil escalating water warming and intensifying heatwaves in the Odra river Basin, Central Europe 长期日水温揭示了中欧奥德拉河流域水温升高和热浪加剧的情况
IF 8.5 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-08-20 DOI: 10.1016/j.gsf.2024.101916
Jiang Sun , Fabio Di Nunno , Mariusz Sojka , Mariusz Ptak , Quan Zhou , Yi Luo , Senlin Zhu , Francesco Granata

Water temperature is a critical indicator and weathervane of aquatic ecosystems. However, the vast majority of rivers lack long-term continuous and complete water temperature datasets. In this study, ensemble models by combining NARX (nonlinear autoregressive network with exogenous inputs) and air2stream were used to reconstruct daily river water temperatures for 27 hydrological stations in the Odra River Basin, one of the largest river systems in Europe. For each hydrological station, both the NARX and air2stream models were calibrated and validated, and the better-performed model was selected to reconstruct daily river water temperatures from 1985 to 2022. The results showed that hybrid modeling by combining NARX and air2stream is promising for reconstructing daily river water temperatures. Based on the reconstructed dataset, annual and seasonal trends of water temperature and characteristics of river heatwaves were evaluated. The results indicated that annual river water temperatures showed a consistent warming trend over the past 40 years with an average warming rate of 0.315 °C/decade. Seasonal river water temperatures indicated that summer warms faster, followed by autumn and spring, and winter river water temperatures showed an insignificant warming trend. River heatwaves are increased in frequency, duration, and intensity in the Odra River Basin, and 6 out of 27 hydrological stations have river heatwaves categorized as ‘severe’ and ‘extreme’, suggesting that mitigation measures are needed to reduce the impact of climate warming on aquatic systems. Moreover, results showed that air temperature is the major controller of river heatwaves, and river heatwaves tend to intensify with the warming of air temperatures.

水温是水生生态系统的重要指标和风向标。然而,绝大多数河流都缺乏长期连续和完整的水温数据集。本研究采用 NARX(具有外生输入的非线性自回归网络)和 air2stream 组合模型,重建了欧洲最大河流系统之一奥德拉河流域 27 个水文站的每日河流水温。对每个水文站的 NARX 模型和 air2stream 模型都进行了校准和验证,并选择性能较好的模型来重建 1985 年至 2022 年的每日河流水温。结果表明,结合 NARX 和 air2stream 的混合模型在重建河流日水温方面具有良好的前景。根据重建的数据集,评估了水温的年度和季节变化趋势以及河流热浪的特征。结果表明,在过去 40 年中,河流年水温呈持续变暖趋势,平均变暖速率为 0.315 ℃/十年。季节性河流水温表明,夏季变暖较快,其次是秋季和春季,冬季河流水温变暖趋势不明显。奥德拉河流域的河流热浪在频率、持续时间和强度上都有所增加,27 个水文站中有 6 个将河流热浪归类为 "严重 "和 "极端",这表明需要采取减缓措施来减少气候变暖对水生系统的影响。此外,研究结果表明,气温是河流热浪的主要控制者,河流热浪往往随着气温的升高而加剧。
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引用次数: 0
Carbon isotope fractionation during methane transport through tight sedimentary rocks: Phenomena, mechanisms, characterization, and implications 甲烷通过致密沉积岩迁移过程中的碳同位素分馏:现象、机制、特征和影响
IF 8.5 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2024-08-10 DOI: 10.1016/j.gsf.2024.101912
Wenbiao Li , Jun Wang , Chengzao Jia , Shuangfang Lu , Junqian Li , Pengfei Zhang , Yongbo Wei , Zhaojing Song , Guohui Chen , Nengwu Zhou

The phenomenon of carbon isotopic fractionation, induced by the transport of methane in tight sedimentary rocks through processes primarily involving diffusion and adsorption/desorption, is ubiquitous in nature and plays a significant role in numerous geological and geochemical systems. Consequently, understanding the mechanisms of transport-induced carbon isotopic fractionation both theoretically and experimentally is of considerable scientific importance. However, previous experimental studies have observed carbon isotope fractionation phenomena that are entirely distinct, and even exhibit opposing characteristics. At present, there is a lack of a convincing mechanistic explanation and valid numerical model for this discrepancy. Here, we performed gas transport experiments under different gas pressures (1–5 MPa) and confining pressures (10–20 MPa). The results show that methane carbon isotope fractionation during natural gas transport through shale is controlled by its pore structure and evolves regularly with increasing effective stress. Compared with the carbon isotopic composition of the source gas, the initial effluent methane is predominantly depleted in 13C, but occasionally exhibits 13C enrichment. The carbon isotopic composition of effluent methane converges to that of the source gas as mass transport reaches a steady state. The evolution patterns of the isotope fractionation curve, transitioning from the initial non-steady state to the final steady state, can be categorized into five distinct types. The combined effect of multi-level transport channels offers the most compelling mechanistic explanation for the observed evolution patterns and their interconversion. Numerical simulation studies demonstrate that existing models, including the Rayleigh model, the diffusion model, and the coupled diffusion-adsorption/desorption model, are unable to describe the observed complex isotope fractionation behavior. In contrast, the multi-scale multi-mechanism coupled model developed herein, incorporating diffusion and adsorption/desorption across multi-level transport channels, effectively reproduces all the observed fractionation patterns and supports the mechanistic rationale for the combined effect. Finally, the potential carbon isotopic fractionation resulting from natural gas transport in/through porous media and its geological implications are discussed in several hypothetical scenarios combining numerical simulations. These findings highlight the limitations of carbon isotopic parameters for determining the origin and maturity of natural gas, and underscore their potential in identifying greenhouse gas leaks and tracing sources.

甲烷在致密沉积岩中通过主要涉及扩散和吸附/解吸的迁移过程而引起的碳同位素分馏现象在自然界无处不在,并在众多地质和地球化学系统中发挥着重要作用。因此,从理论和实验两方面了解迁移诱导碳同位素分馏的机制具有相当重要的科学意义。然而,以往的实验研究观察到的碳同位素分馏现象完全不同,甚至表现出截然相反的特征。目前,这种差异还缺乏令人信服的机理解释和有效的数值模型。在此,我们进行了不同气体压力(1-5 兆帕)和约束压力(10-20 兆帕)下的气体传输实验。结果表明,天然气在页岩中传输过程中的甲烷碳同位素分馏受页岩孔隙结构的控制,并随着有效应力的增加而有规律地变化。与源气的碳同位素组成相比,最初流出的甲烷主要是 13C 贫化,但偶尔也会出现 13C 富化。当质量迁移达到稳定状态时,流出甲烷的碳同位素组成趋同于源气体的碳同位素组成。从初始非稳定状态过渡到最终稳定状态的同位素分馏曲线演变模式可分为五种不同类型。多级传输通道的综合效应为观测到的演变模式及其相互转换提供了最有说服力的机理解释。数值模拟研究表明,现有模型,包括瑞利模型、扩散模型和扩散-吸附/解吸耦合模型,都无法描述观测到的复杂同位素分馏行为。与此相反,本文开发的多尺度多机制耦合模型结合了多级传输通道中的扩散和吸附/解吸作用,有效地再现了所有观测到的分馏模式,并支持综合效应的机制原理。最后,结合数值模拟,讨论了天然气在多孔介质中/通过多孔介质传输时可能产生的碳同位素分馏及其地质影响。这些发现凸显了碳同位素参数在确定天然气来源和成熟度方面的局限性,并强调了其在识别温室气体泄漏和追踪来源方面的潜力。
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