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Spatiotemporal evolution of aeolian sedimentary landscapes on the southern Tibetan Plateau during the late Quaternary: A review and recent advances
IF 10.8 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-02-01 DOI: 10.1016/j.earscirev.2024.105035
Junhuai Yang , Shengqian Chen , Zhiyong Ling , Canyi Zhang , Linkai Wang , Haoyu Wang , Shuyuan Wang , Fuyuan Gao , Ivan Lizaga , Fei Wang , Shengli Yang , Fahu Chen
<div><div>The aeolian deposits on the southern Tibetan Plateau (TP) are one of the most important environmental archives preserved at the highest altitudes worldwide, containing extensive information about both the current and past landscapes and environments of Earth's Third Pole. Over the past three decades, these deposits have attracted considerable attention in Quaternary paleoclimate research. Nevertheless, our understanding of these high-altitude aeolian deposits is significantly less than that for similar deposits in the low-altitude regions of the Eurasian continent. To better comprehend this important archive, it is essential to integrate knowledge from various perspectives. However, there is a lack of consensus regarding their formation, distribution, chronology, provenance, and paleoclimatic history across different timescales. Here, based on our recent field investigations and new data, along with previously published data, we present the results of a systematic analysis of aeolian deposits on the southern TP. Our principal results and findings are: (1) We present up-to-date maps of the aeolian deposits, consisting of an overview map of the overall spatial distribution, and six high-resolution regional maps highlighting details of the depositional areas. Loess and sand dunes have accumulated within the six subdomains, following the global pattern of dust accumulation along rivers in arid and semi-arid regions. (2) Based on paleomagnetic and ESR dating, the oldest aeolian sediments were formed during the middle Pleistocene. The probability density of 220 OSL and AMS <sup>14</sup>C ages reveals that 98.7 % of the young sediments accumulated since the last interglacial, with the majority (66.4 %) forming during the Holocene. A comparison of age clusters with records of ice volume, temperature, precipitation, vegetation, and paleolakes revises previous hypotheses regarding the factors influencing dust deposition, emphasizing the dominant control of climate change. (3) The aeolian sediments are of local origin and their sources remained relatively stable over time. Quantitative analysis of 48 samples using geochemical fingerprinting showed that the aeolian sediments are a mixture of various clastic materials derived from upstream areas, with the predominant contribution from sand dunes (58.7 %). (4) We examined the climatic evolution of this region and its driving mechanisms during the middle to late Pleistocene and the Holocene. This analysis suggests that changes in cold and warm season insolation were the primary external drivers of moisture and dust activity on both orbital and sub-orbital scales. The winter mid-latitude Westerlies and the Indian summer monsoon, which are influenced by these seasonal insolation variations, regulated the moisture evolution, while the near-surface winds, primarily driven by cold season insolation and influenced by ice volume and oscillations in North Atlantic climate, played a significant role in modulat
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引用次数: 0
Terminal Ediacaran–Terreneuvian revolutions in Siberia
IF 10.8 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-02-01 DOI: 10.1016/j.earscirev.2024.105009
Vasiliy V. Marusin
The global reorganizations of marine ecosystems in the terminal Ediacaran and Terreneuvian include two breakthroughs (Cambrian Information Revolution and Agronomic Revolution) followed by the Cambrian Substrate Revolution in the Cambrian Series 2–Furongian. The first two attribute to colonization of new ecological niches by burrowing bilaterians and their gradual expansion within the marine realm. The ichnological record of siliciclastic sequences shows that these processes were most intense in the offshore zone, as compared to more proximal and distal shelf successions. For carbonate basins, the spatial and temporal dynamics of these two revolutions are still poorly understood. The Siberian Platform around the Precambrian–Cambrian transition shows a wide distribution of the marine carbonate facies and hence has high potential for studying the associated endobenthic ecosystem transformations. This study summarizes the results of paleoichnological studies in the terminal Ediacaran and Terreneuvian strata (∼550–521 Ma) in nine regions of the Siberian Platform periphery. The ichnoassemblages are grouped in three stratigraphic intervals (terminal Ediacaran, Fortunian Stage, Cambrian Stage 2) and attributed to sedimentary environments within the models of siliciclastic shelf and/or carbonate ramp. The evolution of the ichnoassemblage structure is evaluated applying the ecosystem engineering and ecospace occupation analyses. The study reveals that the terminal Ediacaran fossil record of the Siberian Platform lacks undisputed trace fossils. In the Terreneuvian, the general patterns of spatiotemporal development of endobenthic communities in the carbonate-associated marine environments generally coincided with those in the siliciclastic basins. The study shows that the greatest innovations in the organism-sediment interactions attributed to the first two Cambrian revolutions happened near the beginning of the Fortunian Stage and Cambrian Stage 2, respectively. However, some important interactions typical for the Agronomic Revolution (e.g., deep infaunal tiering, spreiten burrows) first appeared during the Fortunian.
{"title":"Terminal Ediacaran–Terreneuvian revolutions in Siberia","authors":"Vasiliy V. Marusin","doi":"10.1016/j.earscirev.2024.105009","DOIUrl":"10.1016/j.earscirev.2024.105009","url":null,"abstract":"<div><div>The global reorganizations of marine ecosystems in the terminal Ediacaran and Terreneuvian include two breakthroughs (Cambrian Information Revolution and Agronomic Revolution) followed by the Cambrian Substrate Revolution in the Cambrian Series 2–Furongian. The first two attribute to colonization of new ecological niches by burrowing bilaterians and their gradual expansion within the marine realm. The ichnological record of siliciclastic sequences shows that these processes were most intense in the offshore zone, as compared to more proximal and distal shelf successions. For carbonate basins, the spatial and temporal dynamics of these two revolutions are still poorly understood. The Siberian Platform around the Precambrian–Cambrian transition shows a wide distribution of the marine carbonate facies and hence has high potential for studying the associated endobenthic ecosystem transformations. This study summarizes the results of paleoichnological studies in the terminal Ediacaran and Terreneuvian strata (∼550–521 Ma) in nine regions of the Siberian Platform periphery. The ichnoassemblages are grouped in three stratigraphic intervals (terminal Ediacaran, Fortunian Stage, Cambrian Stage 2) and attributed to sedimentary environments within the models of siliciclastic shelf and/or carbonate ramp. The evolution of the ichnoassemblage structure is evaluated applying the ecosystem engineering and ecospace occupation analyses. The study reveals that the terminal Ediacaran fossil record of the Siberian Platform lacks undisputed trace fossils. In the Terreneuvian, the general patterns of spatiotemporal development of endobenthic communities in the carbonate-associated marine environments generally coincided with those in the siliciclastic basins. The study shows that the greatest innovations in the organism-sediment interactions attributed to the first two Cambrian revolutions happened near the beginning of the Fortunian Stage and Cambrian Stage 2, respectively. However, some important interactions typical for the Agronomic Revolution (e.g., deep infaunal tiering, spreiten burrows) first appeared during the Fortunian.</div></div>","PeriodicalId":11483,"journal":{"name":"Earth-Science Reviews","volume":"261 ","pages":"Article 105009"},"PeriodicalIF":10.8,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143136849","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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
Dispersed organic matter from pre-Devonian marine shales: A review on its composition, origin, evolution, and potential for hydrocarbon prospecting
IF 10.8 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-02-01 DOI: 10.1016/j.earscirev.2024.105027
Qingyong Luo , Fariborz Goodarzi , Ningning Zhong , Nansheng Qiu , Xiaomei Wang , Václav Suchý , Imran Khan , Xiaowei Zheng , Bei Liu , Omid H. Ardakani , Ye Zhang , Dahua Li , Jin Wu , Zilong Fang , Ruitan Shi , Christian B. Skovsted , Hamed Sanei , Yaohui Xu , Jia Wu , Wenxin Hu , Guoqiang Duan
The pre-Devonian shales are important natural archives, preserving extensive information on paleobiology, paleoenvironment, and paleoecology, and also acting as important hydrocarbon source rocks for both unconventional and conventional petroleum systems. In China, however, most of the pre-Devonian shales are postmature, resulting in a gradual convergence in the chemical composition and structure of organic matter (OM). This convergence complicates OM identification under optical microscope, making it challenging to trace its genesis and evolution due to similar optical characteristics. Additionally, the absence of true vitrinite particles poses an additional challenge in the evaluation of thermal maturity of these shales, a challenge that has persisted for decades. This study compares detailed optical characteristics and genesis of selected OM types, namely, graptolite, vitrinite-like maceral (VLM), solid bitumen (SB) in the pre-Devonian shales to improve identification and differentiation between these macerals. The physicochemical evolution of OM is reviewed based on the naturally and artificially matured samples, with emphasis on the organic petrology and petroleum production in some of the most extensively studied pre-Devonian shales globally. VLM and graptolites exhibit higher reflectance and stronger anisotropy than co-occurring in-source SB, with their reflectance as indicators to evaluate OM maturity in these marine shales. VLM can be distinguished from SB by its elongate and syndepositional occurrence, and from graptolites by the characteristic biological structures of graptolite. The origin of VLM is hypothesized to be a product of early diagenetic anaerobic biodegradation of lamalginite and/or bituminite in the Precambrian shales, although its origin in the Cambrian shales remains unclear. On the other hand, in-source SB is derived from the transformation of liptinites or from the cracking of the residual petroleum, or a combination thereof. Graptolites are associated with high total organic carbon (TOC), S1, S2, and hydrogen index (HI) contents, with kerogen predominantly classified as Type II-III, indicating significant hydrocarbon generation potential. Notably, in-source SB plays a significant role in gas generation. In the early mature pre-Devonian shales, OM mainly consists of lamalginite and bituminite; whereas in-source SB becomes the dominant OM in the postmature pre-Devonian shales. Non-granular graptolites are commonly observed in the Ordovician-Silurian Wufeng–Longmaxi shales, contributing significantly to OM. A comparison of naturally and artificially matured samples suggests that low-maturity liptinites transform into SB as thermal maturity increases. This finding is essential for reconstructing the original composition and hydrocarbon potential of these economically significant marine shales.
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引用次数: 0
Seismic hazard and shifting channels: Exploring coseismic river response
IF 10.8 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-02-01 DOI: 10.1016/j.earscirev.2025.105042
Erin McEwan , Timothy Stahl , Rob Langridge , Tim Davies , Andrew Howell , Matthew Wilson
<div><div>Large earthquakes can trigger cascading flood hazards that can influence societal risk and loss; however, the mechanisms driving coseismic river response (CRR) in seismogenic regions have not been fully characterized. This review synthesizes data from fifty-two global cases of CRR where surface deformation affected rivers and identifies the key physical and environmental parameters that control riverine flood hazard in earthquakes. We identify four primary CRR classes, ranging from channel-confined ponding to overbank flooding and avulsion, wherein a river shifts into an enduring new course within the floodplain. CRR susceptibility governs the likelihood, spatial extent, and longevity of CRR, and links back to the characteristics of the surface deformation, river planform, and host environmental setting. Dip-slip fault ruptures, with a large vertical separation at the surface capable of damming river channels, are the primary driver of CRR. Multi-meter dip-slip offsets are also linked to fault-block tilting, which reduce or reverse the gradients of overlying channels. These tilted fault blocks can induce coseismic flooding or avulsion away from the principal fault, with cases documented up c. 10 km upstream from the fault-river intersection. Lateral offsets can amplify or modulate CRR but are generally less effective than vertical offsets at causing them. Two-thirds of CRR cases occurred in single-thread rivers, the majority of which are meandering systems occupying intermontane or lowland basins. Liquefaction-prone substrates in these floodplains exacerbate CRR impacts through ground deformation that disrupts river channel profiles and the local water table. Overbank flooding, lake formation, and prolonged surface flooding are common outcomes near meandering channels and may occur away from the principal fault. Confined braided rivers with high width-to-depth ratios are more resistant to overbank flow and avulsion. In unconfined settings, erodible substrates, and low lateral bank stability amplify the potential for channel scour and rapid avulsion. Braided floodplains often host dense networks of paleochannels within their floodplain, and in any environment, paleochannels enhance the potential for, and geographic extent of flooding and avulsion. High discharge conditions elevate the potential for overbank flow and avulsion, and the hazard posed by CRR may be higher in regions where the climate is perennially or seasonally wet. The risk posed by CRR during earthquakes is heightened in areas where population expansion and land reclamation in flood and liquefaction-prone zones is commonplace. A method to assess CRR risk in advance is required, and a probabilistic framework incorporating uncertainties in fault behaviour, recurrence intervals, and flood-rating curves may offer a way to evaluate absolute hazard in areas where faults and rivers intersect. Site-specific hydrodynamic modelling can further quantify potential changes in flood pat
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引用次数: 0
The deterioration and collapse of late Permian marine ecosystems and the end-Permian mass extinction: A global view
IF 10.8 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-02-01 DOI: 10.1016/j.earscirev.2024.104971
Weihong He , G.R. Shi , Kexin Zhang , N. Suzuki , Han Wang , Fangfang Yang , Yifan Xiao , Tinglu Yang , Yafei Huang , Chen Wu , Ke Jiang
An ever-expanding body of studies has revealed that the evolution of late Permian ecosystems was very complex and possibly involved some yet under-studied ‘early warning signals’ prior to the end-Permian mass extinction. However, the evidence in support of pre-extinction ‘warning signals’ is still limited. In a global review, this paper examined the timing for the initial and peak stages of the late Permian (including the Permian-Triassic boundary interval) biodiversity crisis across different palaeogeographic (palaeobathymetric) settings ranging from pelagic, deep-water basin/deep shelf, through moderately deep-water slope, and to shallow-water carbonate, reef and shallow shelf settings. Based on detailed correlations of globally significant Permian-Triassic sections (20 key sections reviewed) and key stratigraphic boundaries using bio-, chrono- and chemo-stratigraphy, this paper evaluated, summarized and compared the timing and pacing of the environmental and ecosystem deterioration processes in each and among the different palaeogeographic settings and between planktons (mainly radiolarians) and benthos (represented mainly by brachiopods and benthic foraminifers) in deep and moderately deep marine waters. Additionally, where data available we also reviewed the temporal evolution of redox conditions for 17 Permian-Triassic key sections in an attempt to ascertain if there were any notable temporal correlations between these two seemingly separate but potentially mechanistically linked processes. Finally, we also discussed the possible cause-effect and mutually amplifying relationships among volcanism, warming, dynamics of the oxygen minimum zone (OMZ), and the deterioration and final collapse of both marine and terrestrial ecosystems in the late Permian in the lead up to the end-Permian mass extinction.
{"title":"The deterioration and collapse of late Permian marine ecosystems and the end-Permian mass extinction: A global view","authors":"Weihong He ,&nbsp;G.R. Shi ,&nbsp;Kexin Zhang ,&nbsp;N. Suzuki ,&nbsp;Han Wang ,&nbsp;Fangfang Yang ,&nbsp;Yifan Xiao ,&nbsp;Tinglu Yang ,&nbsp;Yafei Huang ,&nbsp;Chen Wu ,&nbsp;Ke Jiang","doi":"10.1016/j.earscirev.2024.104971","DOIUrl":"10.1016/j.earscirev.2024.104971","url":null,"abstract":"<div><div>An ever-expanding body of studies has revealed that the evolution of late Permian ecosystems was very complex and possibly involved some yet under-studied ‘early warning signals’ prior to the end-Permian mass extinction. However, the evidence in support of pre-extinction ‘warning signals’ is still limited. In a global review, this paper examined the timing for the initial and peak stages of the late Permian (including the Permian-Triassic boundary interval) biodiversity crisis across different palaeogeographic (palaeobathymetric) settings ranging from pelagic, deep-water basin/deep shelf, through moderately deep-water slope, and to shallow-water carbonate, reef and shallow shelf settings. Based on detailed correlations of globally significant Permian-Triassic sections (20 key sections reviewed) and key stratigraphic boundaries using bio-, chrono- and chemo-stratigraphy, this paper evaluated, summarized and compared the timing and pacing of the environmental and ecosystem deterioration processes in each and among the different palaeogeographic settings and between planktons (mainly radiolarians) and benthos (represented mainly by brachiopods and benthic foraminifers) in deep and moderately deep marine waters. Additionally, where data available we also reviewed the temporal evolution of redox conditions for 17 Permian-Triassic key sections in an attempt to ascertain if there were any notable temporal correlations between these two seemingly separate but potentially mechanistically linked processes. Finally, we also discussed the possible cause-effect and mutually amplifying relationships among volcanism, warming, dynamics of the oxygen minimum zone (OMZ), and the deterioration and final collapse of both marine and terrestrial ecosystems in the late Permian in the lead up to the end-Permian mass extinction.</div></div>","PeriodicalId":11483,"journal":{"name":"Earth-Science Reviews","volume":"261 ","pages":"Article 104971"},"PeriodicalIF":10.8,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143136874","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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
Molecular mechanisms and biomineralization processes of ferromanganese nodule formation: Insights its effect on nutrient imbalance and heavy metal immobilization in native soil profiles 锰铁结核形成的分子机制和生物矿化过程:对原生土壤养分失衡和重金属固定化的影响
IF 10.8 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-02-01 DOI: 10.1016/j.earscirev.2024.105029
Danish Ali , Suprokash Koner , Ashiq Hussain , Bing-Mu Hsu
Ferromanganese nodules (FMNs), simultaneously termed as manganese nodules, are metallic concretions typically found in the B horizon of iron and manganese-rich soils. These nodules are primarily formed through the biomineralization process driven by favorable redox reactions and microbial activity. The formation of FMNs in the soil is governed by complex geochemical interactions and influenced by both biotic and abiotic factors, such as temperature, pH, organic matter, redox potential (Eh), wet/dry cycles, and nucleation sites. FMNs typically vary in size, ranging from a few microns to several centimeters, and exhibit diverse shapes, from spherical to irregular. These nodules play a crucial role in nutrient cycling and the adsorption of heavy metals, including phosphorus, lead, copper, zinc, cobalt, and nickel, thereby improving soil quality and preventing metal leaching into aquatic environments. The ion exchange during redox reactions, complexation, occlusion, and adsorption are the key mechanisms through which heavy metals can become immobilized in soil FMNs. The formation of FMNs involves Mn-oxidizing bacteria, such as Bacillus, Pedomicrobium, Erythrobacter, Pseudomonas putida, Geobacter, and Leptothrix discophora, which use specific functional genes such as mnxG, moxA, mopA, CumA, ombB, omaB, OmcB, and mofA to facilitate manganese oxidation. This process reacts with geological material, resulting in the precipitation of metal leachates and the development of metal oxide coatings that serve as nucleation sites for FMNs. Such microbial activities are not only essential for FMNs formation but also for trapping heavy metals in soil, highlighting their importance in soil biogeochemical cycling and ecological functions. However, further research is needed to unravel the complex biogeochemical interactions that influence FMNs growth and composition, as well as to understand the stabilization and release dynamics of nutrients and heavy metals, and the roles of microbial communities and functional genes involved in these processes, particularly in relation to soil fertility and plant nutrition.
锰铁结核(FMNs),又称锰结核,是富铁和富锰土壤B层中常见的金属结核。这些结核主要是通过有利的氧化还原反应和微生物活性驱动的生物矿化过程形成的。土壤中FMNs的形成受复杂的地球化学相互作用控制,并受到温度、pH、有机质、氧化还原电位(Eh)、干湿循环和成核位置等生物和非生物因素的影响。fmn通常大小不等,从几微米到几厘米不等,形状各异,从球形到不规则。这些根瘤在养分循环和对磷、铅、铜、锌、钴和镍等重金属的吸附中起着至关重要的作用,从而改善土壤质量,防止金属浸出到水生环境中。氧化还原反应中的离子交换、络合、封闭和吸附是重金属在土壤中固定化的关键机制。FMNs的形成涉及到锰氧化细菌,如芽孢杆菌、Pedomicrobium、红杆菌、恶臭假单胞菌、Geobacter和discophora Leptothrix等,它们利用mnxG、moxA、mopA、CumA、ombB、omaB、OmcB和mofA等特定功能基因促进锰氧化。这个过程与地质物质发生反应,导致金属渗滤液的沉淀和金属氧化物涂层的发展,作为fmn的成核点。这些微生物活动不仅对FMNs的形成至关重要,而且对土壤中重金属的捕获至关重要,突出了它们在土壤生物地球化学循环和生态功能中的重要性。然而,需要进一步的研究来揭示影响FMNs生长和组成的复杂生物地球化学相互作用,了解养分和重金属的稳定和释放动力学,以及参与这些过程的微生物群落和功能基因的作用,特别是与土壤肥力和植物营养有关的作用。
{"title":"Molecular mechanisms and biomineralization processes of ferromanganese nodule formation: Insights its effect on nutrient imbalance and heavy metal immobilization in native soil profiles","authors":"Danish Ali ,&nbsp;Suprokash Koner ,&nbsp;Ashiq Hussain ,&nbsp;Bing-Mu Hsu","doi":"10.1016/j.earscirev.2024.105029","DOIUrl":"10.1016/j.earscirev.2024.105029","url":null,"abstract":"<div><div>Ferromanganese nodules (FMNs), simultaneously termed as manganese nodules, are metallic concretions typically found in the B horizon of iron and manganese-rich soils. These nodules are primarily formed through the biomineralization process driven by favorable redox reactions and microbial activity. The formation of FMNs in the soil is governed by complex geochemical interactions and influenced by both biotic and abiotic factors, such as temperature, pH, organic matter, redox potential (Eh), wet/dry cycles, and nucleation sites. FMNs typically vary in size, ranging from a few microns to several centimeters, and exhibit diverse shapes, from spherical to irregular. These nodules play a crucial role in nutrient cycling and the adsorption of heavy metals, including phosphorus, lead, copper, zinc, cobalt, and nickel, thereby improving soil quality and preventing metal leaching into aquatic environments. The ion exchange during redox reactions, complexation, occlusion, and adsorption are the key mechanisms through which heavy metals can become immobilized in soil FMNs. The formation of FMNs involves Mn-oxidizing bacteria, such as <em>Bacillus, Pedomicrobium, Erythrobacter, Pseudomonas putida, Geobacter,</em> and <em>Leptothrix discophora,</em> which use specific functional genes such as <em>mnxG, moxA, mopA, CumA, ombB, omaB, OmcB,</em> and <em>mofA</em> to facilitate manganese oxidation. This process reacts with geological material, resulting in the precipitation of metal leachates and the development of metal oxide coatings that serve as nucleation sites for FMNs. Such microbial activities are not only essential for FMNs formation but also for trapping heavy metals in soil, highlighting their importance in soil biogeochemical cycling and ecological functions. However, further research is needed to unravel the complex biogeochemical interactions that influence FMNs growth and composition, as well as to understand the stabilization and release dynamics of nutrients and heavy metals, and the roles of microbial communities and functional genes involved in these processes, particularly in relation to soil fertility and plant nutrition.</div></div>","PeriodicalId":11483,"journal":{"name":"Earth-Science Reviews","volume":"261 ","pages":"Article 105029"},"PeriodicalIF":10.8,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142874281","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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
A systematic review of the hydrogeomorphological impacts of large dams in Africa
IF 10.8 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-01-27 DOI: 10.1016/j.earscirev.2025.105048
Sofie Annys , Amaury Frankl
Large dams exert significant impacts on the hydrology and geomorphology of the rivers they impound. Although there is a renewed interest in large dams in Africa to support sustainable development in the face of a changing climate, no systematic review of their hydrogeomorphological impacts exists at continental scale. In this review, we compiled a geospatial dataset of 1047 large dams from different data sources (jointly storing up to 948.7 km3; equal to 29 % of the continent's average annual discharge), and systematically investigated the impact these dams have on water and sediment regimes, river and coastal geomorphology. Our findings reveal a consistent augmentation in low flows and a pronounced reduction in high flows (resulting in an average 35 % reduction in the coefficient of variation of monthly discharges), and often, a decrease in average river flows. The total sediment retention by these dams was estimated at 459.6 Mt. yr-1, with fluxes towards the Mediterranean Sea being particularly reduced by 197.6 Mt. yr-1. Although trends in altered flow regimes and trapping efficiencies (average of 85.5 %) display broad consistency across the continent, the associated geomorphological changes frequently exhibit localized variations. Common alterations encompass riverbed incision and a narrowing of the active riverbed. Coastal erosion and the permanent opening or closing of estuaries are also recurrently observed. This research significantly advances our understanding of the water infrastructure and its potential challenges for sustainable water and sediment management in the context of a changing climate and ever-high erosion rates.
{"title":"A systematic review of the hydrogeomorphological impacts of large dams in Africa","authors":"Sofie Annys ,&nbsp;Amaury Frankl","doi":"10.1016/j.earscirev.2025.105048","DOIUrl":"10.1016/j.earscirev.2025.105048","url":null,"abstract":"<div><div>Large dams exert significant impacts on the hydrology and geomorphology of the rivers they impound. Although there is a renewed interest in large dams in Africa to support sustainable development in the face of a changing climate, no systematic review of their hydrogeomorphological impacts exists at continental scale. In this review, we compiled a geospatial dataset of 1047 large dams from different data sources (jointly storing up to 948.7 km<sup>3</sup>; equal to 29 % of the continent's average annual discharge), and systematically investigated the impact these dams have on water and sediment regimes, river and coastal geomorphology. Our findings reveal a consistent augmentation in low flows and a pronounced reduction in high flows (resulting in an average 35 % reduction in the coefficient of variation of monthly discharges), and often, a decrease in average river flows. The total sediment retention by these dams was estimated at 459.6 Mt. yr<sup>-1</sup>, with fluxes towards the Mediterranean Sea being particularly reduced by 197.6 Mt. yr<sup>-1</sup>. Although trends in altered flow regimes and trapping efficiencies (average of 85.5 %) display broad consistency across the continent, the associated geomorphological changes frequently exhibit localized variations. Common alterations encompass riverbed incision and a narrowing of the active riverbed. Coastal erosion and the permanent opening or closing of estuaries are also recurrently observed. This research significantly advances our understanding of the water infrastructure and its potential challenges for sustainable water and sediment management in the context of a changing climate and ever-high erosion rates.</div></div>","PeriodicalId":11483,"journal":{"name":"Earth-Science Reviews","volume":"262 ","pages":"Article 105048"},"PeriodicalIF":10.8,"publicationDate":"2025-01-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143180624","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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
Tectono-magmatic controls on porphyry Cu endowment in the Carboniferous Dananhu Arc, Central Asian Orogenic Belt: A review
IF 10.8 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-01-22 DOI: 10.1016/j.earscirev.2025.105047
Yi-Hao Liu , Chun-Ji Xue , Yun Zhao , Xiao-Bo Zhao , Reimar Seltmann , Matthew J. Brzozowski , David T.A. Symons
Situated in the southwestern margin of the Central Asian Orogenic Belt, the Dananhu Arc is a prominent porphyry Cu belt in NW China. The Carboniferous granitoids that host two giant to large and several medium to small porphyry Cu deposits are concentrated in the middle segment of the arc. In contrast, coeval granitoids in the adjacent western and eastern segments are barren. The key factors controlling porphyry fertility and diversity in this arc have not been well constrained. The geochemical and Sr–Nd–Hf–O isotopic compositions of Carboniferous fertile and barren magmas exhibit systematic variations from west to east along the 600 km-long Dananhu Arc. Fertile granitoids have adakitic affinities, with high Sr/Y ratios, Mg#, and oxygen fugacity (ΔFMQ = +2.53 ± 0.52), and depleted Sr–Nd–Hf–O isotopic compositions. The barren alkaline granitoids in the western segment are characterized by enrichments in large ion lithophile elements, low Mg# and oxygen fugacity (ΔFMQ = +0.31 ± 0.11), and evolved Sr–Nd–Hf–O isotope compositions. The barren calc-alkaline granitoids in the eastern segment have low Sr/Y ratios, moderate Mg# and oxygen fugacity (ΔFMQ = +1.65 ± 0.50), and depleted Sr–Nd–Hf–O isotopic compositions. The fertile adakitic granitoids originated from partial melting of a flat-subducted oceanic slab accompanied by crustal thickening. The barren alkaline granitoids were derived from anatexis of accretionary complexes triggered by slab rollback accompanied by magma migration and crustal thinning. The barren calc-alkaline granitoids were derived from partial melting of the mantle wedge in a normal subduction setting. Taken together, we suggest that distinct tectonic settings generated the heterogeneous distribution of porphyry Cu deposits throughout the Dananhu Arc by controlling the nature of the magma that was generated.
{"title":"Tectono-magmatic controls on porphyry Cu endowment in the Carboniferous Dananhu Arc, Central Asian Orogenic Belt: A review","authors":"Yi-Hao Liu ,&nbsp;Chun-Ji Xue ,&nbsp;Yun Zhao ,&nbsp;Xiao-Bo Zhao ,&nbsp;Reimar Seltmann ,&nbsp;Matthew J. Brzozowski ,&nbsp;David T.A. Symons","doi":"10.1016/j.earscirev.2025.105047","DOIUrl":"10.1016/j.earscirev.2025.105047","url":null,"abstract":"<div><div>Situated in the southwestern margin of the Central Asian Orogenic Belt, the Dananhu Arc is a prominent porphyry Cu belt in NW China. The Carboniferous granitoids that host two giant to large and several medium to small porphyry Cu deposits are concentrated in the middle segment of the arc. In contrast, coeval granitoids in the adjacent western and eastern segments are barren. The key factors controlling porphyry fertility and diversity in this arc have not been well constrained. The geochemical and Sr–Nd–Hf–O isotopic compositions of Carboniferous fertile and barren magmas exhibit systematic variations from west to east along the 600 km-long Dananhu Arc. Fertile granitoids have adakitic affinities, with high Sr/Y ratios, Mg#, and oxygen fugacity (ΔFMQ = +2.53 ± 0.52), and depleted Sr–Nd–Hf–O isotopic compositions. The barren alkaline granitoids in the western segment are characterized by enrichments in large ion lithophile elements, low Mg# and oxygen fugacity (ΔFMQ = +0.31 ± 0.11), and evolved Sr–Nd–Hf–O isotope compositions. The barren calc-alkaline granitoids in the eastern segment have low Sr/Y ratios, moderate Mg# and oxygen fugacity (ΔFMQ = +1.65 ± 0.50), and depleted Sr–Nd–Hf–O isotopic compositions. The fertile adakitic granitoids originated from partial melting of a flat-subducted oceanic slab accompanied by crustal thickening. The barren alkaline granitoids were derived from anatexis of accretionary complexes triggered by slab rollback accompanied by magma migration and crustal thinning. The barren calc-alkaline granitoids were derived from partial melting of the mantle wedge in a normal subduction setting. Taken together, we suggest that distinct tectonic settings generated the heterogeneous distribution of porphyry Cu deposits throughout the Dananhu Arc by controlling the nature of the magma that was generated.</div></div>","PeriodicalId":11483,"journal":{"name":"Earth-Science Reviews","volume":"262 ","pages":"Article 105047"},"PeriodicalIF":10.8,"publicationDate":"2025-01-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143180622","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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
Tectonic evolution of the eastern Central Asian Orogenic Belt during the Carboniferous–Permian 石炭纪-二叠纪中亚造山带东部的构造演化
IF 10.8 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-01-21 DOI: 10.1016/j.earscirev.2025.105046
Tong Zhou , Yongjiang Liu , Qingbin Guan , Boran Liu , Wenjiao Xiao , Sanzhong Li , Zhaoxu Chen , A. Yu Peskov
The eastern Central Asian Orogenic Belt (CAOB) is an interactive area of multiple tectonic regimes. In the past decades, researchers have conducted extensive studies in the eastern CAOB over the past decades and reported plenty of new data. However, there are still many open questions and arguments dealing with the correlation and tectonic affinity of different blocks with Precambrian crystalline basements, the subduction tectonic processes, and the initiation time of the oceans surrounding the blocks at the eastern CAOB. In this study, we provide a detailed review of the tectonic evolution of the Precambrian blocks in the Eastern Mongolia, NE China, and Far East Russia and provide a regional comparison and correlation of the different tectonic units in the region, initial subduction of Mongolia–Okhotsk Ocean and Pathalassa Ocean, and set up a tectonic evolution model from Carboniferous to Permian. In the late Early Paleozoic, the Ereendavaa Block in Eastern Mongolia and the Erguna and Jiamusi Blocks in NE China, as well as the Mamyn and Bureya Blocks in the Far East Russia, respectively formed the Ereendavaa–Erguna–Mamyn Block chain (EEMB) and Bureya–Jiamusi–Khanka Block chain (BJKB) were formed and probably connected and constructed a long united block chain. Combined with the geochronological and geochemical data of the late Paleozoic magmatic rocks from these tectonic units, we suggest that the southeastward subduction of the Mongolia–Okhotsk Ocean along the northwestern margin of the EEMB was initiated in the Late Carboniferous, then the westward subduction of the Panthalassa Ocean along the eastern margin of the BJKB was subsequently initiated in the Late Carboniferous, indicating that the initial subduction around outside of which migrated from west to east. With the continuous subduction of the Mongolia–Okhotsk Ocean and Panthalassa Ocean, the EEMB–BJKB block chain underwent further bending, forming a southward–opened curve and constituted the NE China Orocline.
{"title":"Tectonic evolution of the eastern Central Asian Orogenic Belt during the Carboniferous–Permian","authors":"Tong Zhou ,&nbsp;Yongjiang Liu ,&nbsp;Qingbin Guan ,&nbsp;Boran Liu ,&nbsp;Wenjiao Xiao ,&nbsp;Sanzhong Li ,&nbsp;Zhaoxu Chen ,&nbsp;A. Yu Peskov","doi":"10.1016/j.earscirev.2025.105046","DOIUrl":"10.1016/j.earscirev.2025.105046","url":null,"abstract":"<div><div>The eastern Central Asian Orogenic Belt (CAOB) is an interactive area of multiple tectonic regimes. In the past decades, researchers have conducted extensive studies in the eastern CAOB over the past decades and reported plenty of new data. However, there are still many open questions and arguments dealing with the correlation and tectonic affinity of different blocks with Precambrian crystalline basements, the subduction tectonic processes, and the initiation time of the oceans surrounding the blocks at the eastern CAOB. In this study, we provide a detailed review of the tectonic evolution of the Precambrian blocks in the Eastern Mongolia, NE China, and Far East Russia and provide a regional comparison and correlation of the different tectonic units in the region, initial subduction of Mongolia–Okhotsk Ocean and Pathalassa Ocean, and set up a tectonic evolution model from Carboniferous to Permian. In the late Early Paleozoic, the Ereendavaa Block in Eastern Mongolia and the Erguna and Jiamusi Blocks in NE China, as well as the Mamyn and Bureya Blocks in the Far East Russia, respectively formed the Ereendavaa–Erguna–Mamyn Block chain (EEMB) and Bureya–Jiamusi–Khanka Block chain (BJKB) were formed and probably connected and constructed a long united block chain. Combined with the geochronological and geochemical data of the late Paleozoic magmatic rocks from these tectonic units, we suggest that the southeastward subduction of the Mongolia–Okhotsk Ocean along the northwestern margin of the EEMB was initiated in the Late Carboniferous, then the westward subduction of the Panthalassa Ocean along the eastern margin of the BJKB was subsequently initiated in the Late Carboniferous, indicating that the initial subduction around outside of which migrated from west to east. With the continuous subduction of the Mongolia–Okhotsk Ocean and Panthalassa Ocean, the EEMB–BJKB block chain underwent further bending, forming a southward–opened curve and constituted the NE China Orocline.</div></div>","PeriodicalId":11483,"journal":{"name":"Earth-Science Reviews","volume":"262 ","pages":"Article 105046"},"PeriodicalIF":10.8,"publicationDate":"2025-01-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143181198","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"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
Thermally driven organic-inorganic interactions in sedimentary basins: A review from source rocks to reservoirs
IF 10.8 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY Pub Date : 2025-01-20 DOI: 10.1016/j.earscirev.2025.105043
Guanghui Yuan , Yingchang Cao , Zhijun Jin , Hans-Martin Schulz , Zihao Jin , Rui Fang , Xiaoyang Zhao , Keyu Liu , Jixuan Wang
Organic-inorganic interactions, ubiquitous in sedimentary basins, critically influence the genesis and evolution of petroleum and natural gases. These processes also modify the inorganic rock matrix as well as cause the formation of secondary pores. This review synthesizes evidences from thermal experiments and geological case studies to examine the genesis, evolution pathways and significance of thermally driven interactions in kerogen-rich source rocks and hydrocarbon reservoirs.
Several mechanisms have been proposed to elucidate the initiation of these interactions, including the carbonium-ion mechanisms, stepwise-oxidation of hydrocarbon by water in the presence of ferric iron-bearing minerals, Fischer-Tropsch-type (FTT) synthetic reactions, and free radical mechanisms. Recent observations of water microdroplets formed near oil-water interfaces at elevated temperatures suggest a potential non-catalytic free radical mechanism underlying the oil-water interactions in hot hydrocarbon reservoirs. In source rocks, clay minerals (smectite, S/I, and illite), calcite, and Fe/Mn-containing metal minerals significantly impact kerogen degradation through their Brønsted and Lewis acid sites, M2+-O surface groups, and partially filled d orbitals. In reservoir settings, kaolinite, illite, feldspar and carbonate minerals primarily influence hydrocarbon degradation. Water, present throughout these environments, facilitates the generation of low-molecular-weight hydrocarbons, organic acids, and CO2 through external hydrogen and oxygen contribution. It also modulates minerals effects on the thermal evolution of kerogen, crude oil, and natural gases. Acids produced during kerogen maturation promote mineral alterations, including smectite illitization, feldspar alteration and calcite recrystallization. These processes, sustained by continuous acid generation from hydrocarbon oxidation, contribute to ongoing mineral transformation and secondary porosity development in deeply buried reservoirs, significantly affecting reservoir quality. At elevated temperatures, extensive organic-inorganic interactions, facilitated by inorganic-derived hydrogen and oxygen, influence deep hydrocarbon potential, natural gas isotopic composition, and the depth limit of liquid hydrocarbon preservation.
Despite these advances, uncertainties remain regarding the differential impacts of various inorganic species on organic reactions. Future research should focus on elucidating the detailed evolution pathways and associated reactions of thermally altered rocks with diverse organic-inorganic combinations, particularly in fine-grained shales and ultra-deep hydrocarbon reservoirs. Additionally, investigating the quantitative kinetics of coupled mineral alteration and organic reactions would address crucial knowledge gaps in our understanding of these processes.
有机-无机相互作用在沉积盆地中无处不在,对石油和天然气的成因和演化产生了至关重要的影响。这些过程还会改变无机岩石基质,并导致次生孔隙的形成。这篇综述综合了热实验和地质案例研究的证据,探讨了富含角质源岩和碳氢化合物储层中热驱动相互作用的成因、演化路径和意义。有人提出了几种机制来阐明这些相互作用的起因,包括羰离子机制、含铁矿物存在时水对碳氢化合物的逐步氧化、费托合成反应(FTT)和自由基机制。最近对高温下油水界面附近形成的水微滴的观察表明,高温油气藏中油水相互作用的基础是一种潜在的非催化自由基机制。在源岩中,粘土矿物(smectite、S/I 和伊利石)、方解石和含铁/锰的金属矿物通过它们的布氏硬度和路易斯酸位点、M2+-O 表面基团和部分填充的 d 轨道对角质降解产生重大影响。在储层环境中,高岭石、伊利石、长石和碳酸盐矿物主要影响碳氢化合物的降解。水存在于这些环境中,通过外部氢和氧的作用,促进低分子量碳氢化合物、有机酸和二氧化碳的生成。水还能调节矿物对角质、原油和天然气热演化的影响。在角质成熟过程中产生的酸会促进矿物的改变,包括辉石化、长石改变和方解石重结晶。这些过程在碳氢化合物氧化过程中持续产生的酸的作用下,促进了深埋储层中矿物的不断转化和次生孔隙的发育,对储层质量产生了重大影响。在高温条件下,有机物与无机物之间在无机物衍生的氢气和氧气的促进下发生广泛的相互作用,从而影响深层碳氢化合物的潜力、天然气同位素组成以及液态碳氢化合物的保存深度极限。尽管取得了这些进展,但各种无机物对有机反应的不同影响仍存在不确定性。未来的研究应侧重于阐明具有多种有机-无机组合的热蚀变岩石的详细演化路径和相关反应,特别是在细粒页岩和超深层油气藏中。此外,研究矿物蚀变与有机反应耦合的定量动力学将弥补我们在了解这些过程方面的知识空白。
{"title":"Thermally driven organic-inorganic interactions in sedimentary basins: A review from source rocks to reservoirs","authors":"Guanghui Yuan ,&nbsp;Yingchang Cao ,&nbsp;Zhijun Jin ,&nbsp;Hans-Martin Schulz ,&nbsp;Zihao Jin ,&nbsp;Rui Fang ,&nbsp;Xiaoyang Zhao ,&nbsp;Keyu Liu ,&nbsp;Jixuan Wang","doi":"10.1016/j.earscirev.2025.105043","DOIUrl":"10.1016/j.earscirev.2025.105043","url":null,"abstract":"<div><div>Organic-inorganic interactions, ubiquitous in sedimentary basins, critically influence the genesis and evolution of petroleum and natural gases. These processes also modify the inorganic rock matrix as well as cause the formation of secondary pores. This review synthesizes evidences from thermal experiments and geological case studies to examine the genesis, evolution pathways and significance of thermally driven interactions in kerogen-rich source rocks and hydrocarbon reservoirs.</div><div>Several mechanisms have been proposed to elucidate the initiation of these interactions, including the carbonium-ion mechanisms, stepwise-oxidation of hydrocarbon by water in the presence of ferric iron-bearing minerals, Fischer-Tropsch-type (FTT) synthetic reactions, and free radical mechanisms. Recent observations of water microdroplets formed near oil-water interfaces at elevated temperatures suggest a potential non-catalytic free radical mechanism underlying the oil-water interactions in hot hydrocarbon reservoirs. In source rocks, clay minerals (smectite, S/I, and illite), calcite, and Fe/Mn-containing metal minerals significantly impact kerogen degradation through their Brønsted and Lewis acid sites, M<sup>2+</sup>-O surface groups, and partially filled d orbitals. In reservoir settings, kaolinite, illite, feldspar and carbonate minerals primarily influence hydrocarbon degradation. Water, present throughout these environments, facilitates the generation of low-molecular-weight hydrocarbons, organic acids, and CO<sub>2</sub> through external hydrogen and oxygen contribution. It also modulates minerals effects on the thermal evolution of kerogen, crude oil, and natural gases. Acids produced during kerogen maturation promote mineral alterations, including smectite illitization, feldspar alteration and calcite recrystallization. These processes, sustained by continuous acid generation from hydrocarbon oxidation, contribute to ongoing mineral transformation and secondary porosity development in deeply buried reservoirs, significantly affecting reservoir quality. At elevated temperatures, extensive organic-inorganic interactions, facilitated by inorganic-derived hydrogen and oxygen, influence deep hydrocarbon potential, natural gas isotopic composition, and the depth limit of liquid hydrocarbon preservation.</div><div>Despite these advances, uncertainties remain regarding the differential impacts of various inorganic species on organic reactions. Future research should focus on elucidating the detailed evolution pathways and associated reactions of thermally altered rocks with diverse organic-inorganic combinations, particularly in fine-grained shales and ultra-deep hydrocarbon reservoirs. Additionally, investigating the quantitative kinetics of coupled mineral alteration and organic reactions would address crucial knowledge gaps in our understanding of these processes.</div></div>","PeriodicalId":11483,"journal":{"name":"Earth-Science Reviews","volume":"262 ","pages":"Article 105043"},"PeriodicalIF":10.8,"publicationDate":"2025-01-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143180621","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
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Earth-Science Reviews
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