断层崩积楔单片再生法光释光测年:以山西忻定盆地西田探槽为例   总被引：3，自引：0，他引：3  

赵俊香  任俊杰  于慎谔  张世民  丁锐 《现代地质》2011,25(2):356-362

为了研究断层崩积楔各部位沉积物光释光信号晒退情况及崩积楔形成年龄,利用中颗粒石英(63~90μm)单片再生法(SAR)对山西忻定盆地西田探槽断层崩积楔3个部位的4个样品进行光释光(OSL)定年。选择一代表性样品(08-OSL-22)进行等效剂量(DE)、LN/TN、循环比率、回授率与预热温度的关系分析,结果表明预热温度260℃、预热时间10 s为样品最佳预热条件。4个样品的测片循环比率基本在0.9~1.1之间,回授率均小于5%,表明所采用的中颗粒SAR法流程可以很好地校正测量过程中产生的释光感量变化,其等效剂量可信。利用等效剂量分布直方图和累积频率图,发现古地形面和坡积物的样品晒退均匀,崩积层样品则较差。对于晒退较差的样品利用累积频率法得到其等效剂量,从而得到崩积楔的近似年龄。最后获得该期崩积楔的形成年龄为(27.09±0.71)ka。  相似文献   

Seismic response to collapse structures in the Southern North Sea     

Malcolm K. Jenyon 《Marine and Petroleum Geology》1984,1(1):27-36

The presence of probable salt dissolution-associated collapse structures in the North Sea based on the evidence of contemporary seismic data was discussed by Lohmann (1972). Since then, little attention has been paid to them in North Sea literature, although many oil companies will have studies on file. This Paper describes and illustrates a selection of such features in the area from recent seismic data, and suggest a broad classification for them as they are seen on the seismic section, based on mode of origin. Reference will also be made to certain types of carbonate dissolution and collapse effects.  相似文献   

“Source to Sink”: A Review of Tectonics-Erosion-Sedimentation Interactions in the Analogue Experiments of Accretionary WedgeEI北大核心CSCD     

Deng B.  Huang R.  Ma H.  He Y.  Lai D.  Jiang L.  Liu S. 《大地构造与成矿学》2018,(3):431-444

It is believed that the tectonics-erosion-sedimentation interaction in the analogue experiments was essentially improved by the theory of “from source to sink”. In particular, the widespread uplift and exhumation in the western China occurred in Cenozoic can be considered to be a typical natural laboratory in the world. Here we review our current understanding from tectonic sandbox models of tectonics-erosion-sedimentation and their interactions, as well as from natural laboratory. As we known, there are widespread erosion occurred predominantly at hinterland of the accretionary wedge, in contrast to the sedimentation occurred widely at foreland of the wedge. Therefore, fold-and-thrust belts with low syntectonic sedimentation and erosion would evolve in a self-similar fashion to produce a narrow accretionary wedge, while high syntectonic sedimentation and erosion would produce accretionary wedge with very active hinterland thrusts, and a large width. Furthermore, the critically tapered wedge model suggests that the crust-scale thrust-and-fold belts under a horizontal compressive force would come into a self-similar growth of a forward-tapering wedge when it reaches a critical taper angle of the combined angles of the base dip and the wedge slope. Such a process has important influence on the tectonics-erosion- sedimentation and their interactions both in accretionary wedges and their analogue experiments. Although there is a significant similarity between the analogue experiments and natural accretionary wedges in the surface processes of tectonics- erosion-sedimentation and their interactions, it is difficult to get more universal parameters between them. It should be noted that sandbox models of the accretionary wedges in the natural laboratory would improve significantly our understanding of the theory of the tectonics-erosion-sedimentation interactions and “from source to sink”. © 2018, Science Press. All right reserved.  相似文献   

U–Pb geochronology,Sr–Nd isotopic compositions,geochemistry and petrogenesis of Shah Soltan Ali granitoids,Birjand, Eastern Iran     

Mohammad Hassan Karimpour  Azadeh Malekzadeh Shafaroudi  José Francisco Santos  Ryan Mathur  Sara Ribeiro 《Chemie der Erde / Geochemistry》2018,78(3):299-313

The Shah Soltan Ali area (SSA) is located in the eastern part of the Lut Block metallogenic province. In this area different types of sub-volcanic intrusions including diorite porphyry, monzonite porphyry and monzodiorite porphyry have intruded into basaltic and andesitic rocks. Zircon U–Pb dating and field observations indicate that intermediate to mafic volcanic rocks (38.9 Ma) are older than subvolcanic units (38.3 Ma). The subvolcanic intrusions show high-K calc-alkaline to shoshonitic affinity and are metaluminous. Based on mineralogy, high values of magnetic susceptibility [(634 to 3208) × 10^?5 SI], and low initial ⁸⁷Sr/⁸⁶Sr ratios, they are classified as belonging to the magnetite-series of oxidant I-type granitoids and are characterized by an enrichment in LREEs relative to HREEs, with negative Nb, Ti, Zr and Eu anomalies. These granitoids are related to volcanic arc (VAG) and were generated in an active continental margin. Low initial ⁸⁷Sr/⁸⁶Sr ratios (0.7043 to 0.7052) and positive εNd values (+1.48 to +3.82) indicate that the parental magma was derived from mantle wedge. Parental magma was probably formed by low degree of partial melting and metasomatized by slab derived fluids. Then assimilation and fractional crystallization processes (AFC) produced the SSA rocks. This magma during the ascent was contaminated with the crustal material.All data suggest that Middle-Late Eocene epoch magmatism in the SSA area, occurred during subduction of Neo-Tethys Ocean in east of Iran (between Afghan and Lut Blocks).  相似文献   

3-D crustal-scale gravity model of the San Rafael Block and Payenia volcanic province in Mendoza,Argentina     

Daniel Richarte  Marianela Lupari  Agustina Pesce  Silvina Nacif  Mario Gimenez 《地学前缘(英文版)》2018,9(1):239-248

The San Rafael Block(SRB)is part of one of the main retroarc volcanic provinces in southern Central Andes in Mendoza,Argentina.This block is located in the Andean foothills between the orogenic front and foreland basement uplifts of late Miocene age.In order to analyze the geochronological evolution of the Quaternary volcanism in the region,several geologic and geophysical studies have been conducted.Nevertheless,the crust,where the SRB is located,has not been well characterized yet.Based on gravimetric and magnetic data,together with isostatic and elastic thickness analyses,we modeled the crustal structure of the area.Information obtained has allowed us to understand the crust where the SRB and the Payenia volcanic province are located.Bouguer anomalies indicate that the SRB presents higher densities to the North of Cerro Nevado and Moho calculations suggest depths for this block between 40 and 50 km.Determinations of elastic thickness would indicate that the crust supporting the San Rafael Block presents values of approximately 10 km,being enough to support the block loading.However,in the Payenia region,elastic thickness values are close to zero due to the regional temperature increase.  相似文献   

Intrinsic versus extrinsic variability of analogue sand-box experiments – Insights from statistical analysis of repeated accretionary sand wedge experiments     

《Journal of Structural Geology》2015

Analogue models are not perfectly reproducible even under controlled boundary conditions which make their interpretation and application not always straight forward. As any scientific experiment they include some random component which can be influenced both by intrinsic (inherent processes) and extrinsic (boundary conditions, material properties) sources. In order to help in the assessment of analogue model results, we discriminate and quantify the intrinsic versus extrinsic variability of results from “sandbox” models of accretionary wedges that were repeated in a controlled environment. The extrinsic source of variability, i.e. the parameter varied is the nature of the décollement (material, friction and thickness). Experiment observables include geometric properties of the faults (lifetime, spacing, dip) as well as wedge geometry (height, slope, length).For each variable we calculated the coefficient of variance (CV) and quantified the variability as a symmetric distribution (Normal, Laplacian) or asymmetric distribution (Gamma) using a Chi squared test (χ²). Observables like fault dip/back thrust dip (CV = 0.6–0.7/0.2–0.6) are less variable and decrease in magnitude with decreasing basal friction. Variables that are time dependent like fault lifetime (CV = 0.19–0.56) and fault spacing (CV = 0.12 – 0.36) have a higher CV consequently affecting the variability of wedge slope (CV = 0.12–0.33). These observables also increase in magnitude with increasing basal friction. As the mechanical complexity of the evolving wedge increases over time so does the CV and asymmetry of the distribution. In addition, we confirm the repeatability of experiments using an ANOVA test. Through the statistical analysis of results from repeated experiments we present a tool to quantify variability and an alternative method to gaining better insights into the dynamic mechanics of deformation in analogue sand wedges.  相似文献   

水平荷载下单片地下连续墙基础的应变楔模型分析法     

刘云忠  ;戴国亮 《岩土工程技术》2014,(4):172-176

近年来单片地下连续墙被广泛运用于桥梁工程和高层建筑中,但其大部分研究均集中于单片地下连续墙的竖向承载性能试验研究和理论分析,只进行了少量单片墙的水平承载性能试验研究.通过应变楔模型把墙与土之间复杂的三维接触特性简化为一维的弹性地基梁中所需土体的参数,然后按照弹性地基梁的理论计算墙的内力和变形,利用室内模型试验实测数据验证了该算法的合理性.可为类似工程提供依据.  相似文献   

印支期龙门山造山楔推进作用与前陆型礁滩迁移过程研究   总被引：1，自引：0，他引：1  

李勇  颜照坤  苏德辰  刘树根  曹俊兴  李海兵  孙玮  董顺利 《岩石学报》2014,30(3):641-654

马鞍塘期龙门山前陆盆地是印支期造山楔加载于扬子地台西缘而形成的挠曲前陆盆地。根据地表露头、钻孔剖面和地震反射剖面资料,本文通过分析前陆盆地早期前陆缓坡型鲕粒滩-硅质海绵礁组合在时间和空间上的迁移规律,标定了卡尼期龙门山造山楔的推进速率。结果表明:卡尼期马鞍塘组是分布于底部不整合面之上的第一套地层单元,在垂向上前陆型鲕粒滩-硅质海绵礁组合显示为鲕粒灰岩滩-生物碎屑滩-硅质海绵礁灰岩-泥页岩的向上变细的沉积序列,记录了前缘隆起边缘碳酸盐缓坡和海绵礁的构建和淹没过程,反映了在相对海平面的持续上升中鲕粒滩-硅质海绵礁被淹没致死的过程。在横向上,盆地结构显示为西厚东薄,并向西倾斜的不对称盆地,由西向东依次分布了深水盆地、碳酸盐缓坡和海绵礁和浅水滨岸带等沉积物类型,显示了从龙门山造山楔向前陆一侧具有泥页岩向鲕粒滩-硅质海绵礁的变化特征。其中鲕粒滩-硅质海绵礁丘组合发育于15～30m深度的前陆同斜缓坡上,呈面向西的条带状展布,其走向线与龙门山冲断带的走向大致平行。并可将其划分为7个鲕粒滩-硅质海绵礁相带,表明卡尼期硅质海绵礁丘和滩沿底部不整合面向南东方向的前陆缓坡超覆,其超覆线和相带的走向与龙门山冲断带的走向平行,显示了7条硅质海绵礁丘和滩是随着相对海平上升过程而向南东方向的前陆缓坡超覆过程中逐次形成的。卡尼期硅质海绵礁迁移速率为18mm·yr-1,其与龙门山造山楔推进速率(15mm·yr-1)基本一致,表明印支期龙门山逆冲楔推进速率与前陆鲕粒滩-硅质海绵礁丘迁移速率具有明显的耦合关系。据此,本次提出了龙门山前陆盆地早期前陆型碳酸盐缓坡和硅质海绵礁的迁移模式,其形成的过程为:龙门山造山楔于卡尼期初始构造负载于扬子板块西缘,导致了前陆地区的挠曲沉降,形成了前陆盆地,驱动了相对海平面的持续上升,前陆盆地处于欠补偿状态,当相对海平面上升速率与硅质海绵礁生长速率相同时,在15～30m深度的前陆同斜缓坡上发育了鲕粒滩-硅质海绵礁丘组合,随着龙门山造山楔不断地的向前陆地区推进,前陆盆地内相对海平面持续上升,逐次在前陆缓坡上15～30m深度的的位置开启了新的硅质海绵礁群的生长窗,形成了本区卡尼期7条带状展布的鲕粒滩-硅质海绵礁丘组合。因此,硅质海绵礁的淹没过程和迁移过程是龙门山造山楔向扬子克拉通推进过程的沉积响应,显示了在卡尼期-诺利期松潘-甘孜残留洋盆的迅速闭合和逆冲楔构造负载向扬子板块推进的动力学过程。  相似文献   

Aseismic deep subduction of the Philippine Sea plate and slab window     

《Journal of Asian Earth Sciences》2013

We have made great efforts to collect and combine a large number of high-quality data from local earthquakes and teleseismic events recorded by the dense seismic networks in both South Korea and West Japan. This is the first time that a large number of Korean and Japanese seismic data sets are analyzed jointly. As a result, a high-resolution 3-D P-wave velocity model down to 700-km depth is determined, which clearly shows that the Philippine Sea (PHS) plate has subducted aseismically down to ∼460 km depth under the Japan Sea, Tsushima Strait and East China Sea. The aseismic PHS slab is visible in two areas: one is under the Japan Sea off western Honshu, and the other is under East China Sea off western Kyushu. However, the aseismic PHS slab is not visible between the two areas, where a slab window has formed. The slab window is located beneath the center of the present study region where many teleseismic rays crisscross. Detailed synthetic tests were conducted, which indicate that both the aseismic PHS slab and the slab window are robust features. Using the teleseismic data recorded by the Japanese stations alone, the aseismic PHS slab and the slab window were also revealed (Zhao et al., 2012), though the ray paths in the Japanese data set crisscross less well offshore. The slab window may be caused by the subducted Kyushu-Palau Ridge and Kinan Seamount Chain where the PHS slab may be segmented. Hot mantle upwelling is revealed in the big mantle wedge above the Pacific slab under the present study region, which may have facilitated the formation of the PHS slab window. These novel findings may shed new light on the subduction history of the PHS plate and the dynamic evolution of the Japan subduction zone.  相似文献   

楔挡分流结构爆炸损伤特征数值模拟   总被引：1，自引：0，他引：1  

王秀丽  靳毅虎  孟杰  朱思帅 《地震学刊》2013,(6):617-623,630

楔挡分流结构是一种新型的拦挡结构,在灾害防治中发挥着重要作用,对其在爆炸等特殊荷载作用下的损伤进行研究具有重要的意义。使用ANSYS／AUTODYN软件,首先采用光滑粒子流体动力学方法（smoothed particle hy-drodynamics,SPH）和混凝土的RHT（Riede-Hiermater-Thoma）本构,对前人试验模型进行了模拟计算。通过对试验和模拟结果的对比分析,验证了SPH算法和混凝土RHT本构在模拟混凝土介质中爆炸损伤的可行性。然后使用同样的算法和材料本构,建立全尺寸模型,对混凝土楔挡分流拦挡坝坝体内爆炸损伤及应力波传播进行了模拟计算。通过对计算结果的分析,研究了混凝土介质中爆炸成坑的机理,得到了楔挡分流结构在内部爆炸作用下的爆坑形态特征、药柱上下部混凝土损伤特点、破碎区范围。对坝体中冲击波传播及混凝土碎块抛射等问题进行了探索。  相似文献