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东昆仑造山带海西—印支期东昆南前陆盆地构造岩相古地理 总被引:3,自引:0,他引:3
地层相态的恢复对于研究非史密斯地层区沉积盆地的演化过程有着非常重要的意义。在1∶ 2 5万野外地质填图基础上作出了东昆仑造山带东段东昆南前陆盆地晚二叠世至中三叠世构造岩相古地理图 ,该系列图揭示了东昆南前陆盆地在 5个发展阶段中的岩相分布特征和空间上的古地理展布范围 ,即晚二叠世早期东昆南前陆盆地发育的初始阶段、晚二叠世晚期前陆盆地的扩展至短期萎缩阶段、早三叠世早期前陆盆地的再次扩展阶段、早三叠世晚期盆地发育的高峰阶段和中二叠世前陆盆地的萎缩至消亡阶段。东昆南前陆盆地的演化过程在一定程度上反映了构造对沉积的控制作用 相似文献
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Tahmineh Pirnia Emilio Saccani Ghodrat Torabi Marco Chiari Spela Gorican Edoardo Barbero 《地学前缘(英文版)》2020,11(1):57-81
The Nain and Ashin ophiolites consist of Mesozoic melange units that were emplaced in the Late Cretaceous onto the continental basement of the Central-East Iran microcontinent(CEIM).They largely consist of serpentinized peridotites slices;nonetheless,minor tectonic slices of sheeted dykes and pillow lavas-locally stratigraphically associated with radiolarian cherts-can be found in these ophiolitic melanges.Based on their whole rock geochemistry and mineral chemistry,these rocks can be divided into two geochemical groups.The sheeted dykes and most of the pillow lavas show island arc tholeiitic(IAT)affinity,whereas a few pillow lavas from the Nain ophiolites show calc-alkaline(CA)affinity.Petrogenetic modeling based on trace elements composition indicates that both IAT and CA rocks derived from partial melting of depleted mantle sources that underwent enrichment in subduction-derived components prior to melting.Petrogenetic modeling shows that these components were represented by pure aqueous fluids,or sediment melts,or a combination of both,suggesting that the studied rocks were formed in an arc-forearc tectonic setting.Our new biostratigraphic data indicate this arc-forearc setting was active in the Early Cretaceous.Previous tectonic interpretations suggested that the Nain ophiolites formed,in a Late Cretaceous backarc basin located in the south of the CEIM(the so-called Nain-Baft basin).However,recent studies showed that the CEIM underwent a counter-clockwise rotation in the Cenozoic,which displaced the Nain and Ashin ophiolites in their present day position from an original northeastward location.This evidence combined with our new data and a comparison of the chemical features of volcanic rocks from different ophiolites around the CEIM allow us to suggest that the Nain-Ashin volcanic rocks and dykes were formed in a volcanic arc that developed on the northern margin of the CEIM during the Early Cretaceous in association with the subduction,below the CEIM,of a Neo-Tethys oceanic branch that was existing between the CEIM and the southern margin of Eurasia.As a major conclusion of this paper,a new geodynamic model for the Cretaceous evolution of the CEIM and surrounding Neo-Tethyan oceanic basins is proposed. 相似文献
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D. M. Cocârţă S. Neamţu A. M. Reşetar Deac 《International Journal of Environmental Science and Technology》2016,13(8):2025-2036
Human activities have progressively increased in recent years. Consequently, significant environment deterioration resulted. Soils have a particularly varied vulnerability to heavy metal pollution, especially in the vicinity of industrial areas. Heavy metal contamination of soil may induce risks and hazards to humans and the ecosystem, while toxic metals in soil can severely inhibit the biodegradation of organic contaminants. This paper is focused on human health risk assessment from extremely contaminated soil with heavy metals, mainly with carcinogenic elements. The study refers to an agricultural area in the vicinity of an old metallurgical processing industrial facility. The contaminants evaluated in the present paper are beryllium (Be), cadmium (Cd), chromium (Cr), nickel (Ni) and lead (Pb). Contamination level is pointed out through laboratory analysis results of soil samples taken from 0–0.2 m, 0.2–0.4 m soil layers and up to 2.1 m soil depth. Some heavy metal concentrations (Cd, Cr and Pb) exceed the intervention thresholds for sensitive areas, as they are stipulated in the national regulation in Romania. The identified average concentration levels of Cd, CrVI and Pb in the first layer of the investigated land are 23.83, 7.71 and 704.22 mg/kgd.w, respectively. The results show that the potential risk of human health is relevant (higher than the acceptable one after World Health Organization) and a possible solution for the remediation should become a major concern for the investigated area. 相似文献
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The Transylvanian Basin is a mature hydrocarbon province of Romania characterized by two petroleum systems: Mesozoic (thermogenic) and Miocene (biogenic). An extensive outcrop-based sedimentological and micropaleontological study correlated to seismic and well data discusses the elements of the Miocene petroleum system. The facies associations are indicative of alluvial, fandelta, shallow- and deep-marine settings. These are grouped into four different depositional systems (evaporite, mud-carbonate, sand-mud and sand-gravel). Their evolution in time and space shows large differences between various parts of the basin that have important consequences for exploration. 相似文献
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滇东石漠化伴生“红裸土”表层有机质含量与酸碱度关系分析 总被引:1,自引:0,他引:1
对滇东地区石漠化伴生"红裸土"典型发育地带的表层样品的有机质和酸碱度分析表明:"红裸土"表层有机质含量范围为0.60~38.5(g.kg-1),平均值为13.49(g.kg-1);酸碱度在4.20~5.72。不但"红裸土"表层有机质含量低,呈中强酸性,且"红裸土"表层土壤有机质含量与酸碱度成弱正相关。这一特征与同区域有植被覆盖下的表层土壤相反,与其他典型的喀斯特地区土壤表层有相似的变化规律。这些特征说明"红裸土"可能是形成石漠化过程的一个阶段。 相似文献
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The reaction kinetics of the butadinyl radical, C4H, with various hydrocarbons detected in the atmosphere of Titan (methane, ethane, propane, acetylene, ethene and methylacetylene) are studied over the temperature range of 39-298 K using the Rennes CRESU (Cinétique de Réaction en Ecoulement Supersonique Uniforme) apparatus. Kinetic measurements were made using the pulsed laser photolysis—laser induced fluorescence technique. The rate coefficients, except for the reaction with methane, all show a negative temperature dependence and can be fitted with the following expressions over the temperature range of this study: ; ; , , . These expressions are not intended to be physically meaningful but rather to provide an easy way to introduce experimental results in photochemical models. They are only valid over the temperature range of the experiments. Possible channels of these reactions are discussed as well as possible consequences of these results for the production of large molecules and hazes in the atmosphere of Titan. These results should also be considered for the photochemistry of Giant Planets. 相似文献