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101.
近十年来对锆石研究已从早期的U-Pb放射性同位素定年和锆石同位素分析,发展到大量研究锆石的微量元素。锆石微量元素不仅可以作为锆石Ti温度计估算岩浆温度,也可以用来识别锆石及其母岩的岩石类型和成因,区分岩浆熔体或者流体控制的岩浆作用、变质作用、成矿作用等深部作用过程。文中在归纳总结岩浆锆石、变质锆石、热液锆石、碎屑锆石等不同类型锆石的微量元素成分基础上,以青藏高原碰撞后超钾质岩石中产出的锆石为例,系统介绍了超钾质岩石中各类锆石的结构、年龄和微量元素特征,并应用于解释超钾质岩石成因、岩浆源区成分、岩浆演化和上部地壳物质的混染、下地壳加厚和高原隆升之间的关系。  相似文献   
102.
帕米尔弧形构造带是印度-欧亚板块碰撞变形最强烈的地区之一,是研究构造过程、地貌演化以及气候变化及其相互作用的理想场所。本文基于前人的研究成果,对帕米尔弧形构造带新生代构造单元、地貌特征和动力学演化模型进行了总结归纳,包括:主要构造单元的活动起止时间、活动量及活动速率;帕米尔弧形构造带现今的地貌特征(水系和冰川的分布);帕米尔弧形构造带6种主要的地球动力学演化模型的主要样式、优点及限制。论文提出了帕米尔弧形构造带晚新生代构造研究的三个重要的科学问题:精细厘定构造带内部的不同断裂带运动学特征和相互关系;深部地质过程与浅部响应相结合,探讨构造带形成的深部地质过程控制;将构造过程、气候特征与地貌演化作为一个耦合系统开展研究。  相似文献   
103.
亲铜(亲铁)元素在行星增生演化、核幔分异、地幔岩浆过程、壳幔相互作用以及金属矿床成因等领域具有举足轻重的作用。本文从亲铜元素的地球化学性质出发,介绍了"高维度思维"的亲铜元素含量比值及其在地球科学领域的初步应用:①获得同一份样品中不同亲铜元素含量可在一定程度上降低样品的不均一性(块金效应)对含量比值的影响;②Cu/Ag值可以约束不同高温岩浆过程中硫化物固液状态和亲铜元素地球化学性质,进而认识地幔、洋壳和大陆地壳间的联系;③具有不同分配系数的亲铜元素含量的比值可以鉴别岩浆硫化物饱和史,比如通过亲铜元素的分异约束火星陨石母岩浆的硫化物不饱和演化历史;④依据In-Cd-Zn在硅酸盐地球的含量以及它们的相对亲铜亲铁性质,地球主体增生物质已经消失,不能由陨石代表。  相似文献   
104.
ABSTRACT

The Pelona–Orocopia–Rand and related schists of southern California are an archetypal example of an exhumed shallow subduction complex. ‘The schist’ comprises mainly trench materials underthust beneath continental arc rocks during Late Cretaceous–early Cenozoic collision of one or more oceanic plateaux with southern California. The arc-on-trench relationship, without intervening mantle or lowermost crust, implies that significant subduction erosion accompanied shallow subduction. Upsection increases in metamorphic grade (~150 ± 100°C/km) and spatial variations in age and peak temperature provide an ~50 million year long record of tectonic underplating within a cooling system. Evidence for palaeoseismic events in earliest formed and hottest (locally transitional granulite grade) schists provides a possible field-based record of episodic tremor and slow slip events such as detected in several modern shallow subduction zones. Structural ascent of the schist was achieved in distinct Late Cretaceous–early Eocene and late Oligocene–early Miocene extensional pulses, the first during collapse of gravitationally unstable upper plate assemblages and accompanied by trench-directed (top-NE) lower plate extrusion and the second corresponding temporally, spatially, and in character with core complex formation in the SW United States. The line between schist and core complex belts is blurred by the recent discovery of schist within 40 km of the nearest core complex and containing synkinematic Miocene intrusions, a hallmark of SW U.S. core complexes. The history of schist assembly, metamorphism, and exhumation provides the most complete field-based record of thermo-mechanical processes, subduction erosion and tectonic underplating in particular, that operated during a shallow subduction event. Future cross-disciplinary investigations of, and comparisons between, the schist and other possible ancient (e.g. Swakane gneiss, Sanbagawa belt, Qiangtang terrane) and modern (e.g. Cascadia, SW Japan, central Mexico, Chile) shallow subduction zones will yield new insights into the tectonic and petrologic processes that operate within such systems.  相似文献   
105.
新疆吉木萨尔县准页4井钻探施工技术   总被引:1,自引:1,他引:0       下载免费PDF全文
熊虎林  张飞 《探矿工程》2017,44(12):38-42
以新疆吉木萨尔县准页4井钻探工程为背景,从钻井井身结构、钻具组合、泥浆工艺、取心技术措施、井斜控制等方面,简要介绍了页岩气参数井采用石油钻机施工工艺流程。针对施工过程中遇到的大砾径覆盖层钻进、超长裸眼段钻进及钻井漏失等问题,通过采取优化钻具结构、调整泥浆粘切润滑性能、使用桥浆堵漏等技术措施,工程得以顺利完工,各项技术指标满足设计要求。总结了实践经验,可为该区大口径钻井施工提供经验借鉴。  相似文献   
106.
Preliminary studies of the magnitude and frequency of lee side avalanches (grain flows) on a Namib crescentic dune show that the frequency of grain flows for a given segment of the lee face is dependent on the wind speed and sand transport rate for the period preceding their initiation; and the magnitude of the flows as described by their area is inversely proportional to the interval between flows and thus wind speed and sand transport rates. These studies indicate the potential of using a simple digital video camera technique to document the magnitude, frequency and geometry of grain flows on desert sand dunes.  相似文献   
107.
108.
Numerical modelling of rise and fall of a dense layer in salt diapirs   总被引:4,自引:0,他引:4  
Numerical models are used to study the entrainment of a dense anhydrite layer by a diapir. The anhydrite layer is initially horizontally embedded within a viscous salt layer. The diapir is down-built by aggradation of non-Newtonian sediments ( n = 4, constant temperature) placed on the top of the salt layer. Several parameters (sedimentation rate, salt viscosity, perturbation width and stratigraphic position of the anhydrite layer) are studied systematically to understand their role in governing the entrainment of the anhydrite layer. High sedimentation rates during the early stages of the diapir evolution bury the initial perturbation and, thus, no diapir forms. The anhydrite layer sinks within the buried salt layer. For the same sedimentation rate, increasing viscosity of the salt layer decreases the rise rate of the diapir and reduces the amount (volume) of the anhydrite layer transported into the diapir. Model results show that viscous salt is capable of carrying separate blocks of the anhydrite layer to relatively higher stratigraphic levels. Varying the width of the initial perturbation (in our calculations 400–800 m), from which a diapir triggers, shows that wider diapirs can more easily entrain an embedded anhydrite layer than the narrower diapirs. The anhydrite layer is entrained as long as rise rate of the diapir exceeds the descent rate of the denser anhydrite layer. We conclude that the four parameters mentioned above govern the ability of a salt diapir to entrain an embedded dense layer. However, the model results show that the entrained blocks inevitably sink back if the rise rate of the diapir is less than the rate of descent of the anhydrite layer or the diapir is permanently covered by a stiff overburden in case of high sedimentation rates.  相似文献   
109.
Standard data and methods, such as the inversion of seismic and GPS data, have been used extensively to infer the details of the 2004 December 26 earthquake. The unprecedented large size of this event gave the opportunity to modern altimeters to provide the first clear records of a tsunami in deep ocean, therefore allowing us to study the rupture history from an independent perspective. We invert the Jason-1 and Topex–Poseidon altimetry records, considering the new constraints available on the geometry of the fault plane, and taking them into account in a 3-D rupture model. The data are corrected for the non-negligible effect of satellite motion during measurements. Our results show that the rupture propagated over the 1500 km of subduction zone initially identified by the aftershock distribution, with a magnitude of   M w= 9.1  . Our solution compares well with the latitudinal distribution of slip inferred from other data sets, with a maximum of energy release north of Sumatra, and two other slip patches near the Nicobar and Andaman islands. Based on waveform comparison, we assert that the shallow portion of the megathrust offshore Banda Aceh had slip amplitudes of more than 20 m. Also, we find that significant amounts of slip (about 10 m) concentrated below the Andaman islands and did not propagate on the shallow portion of the interface. Although synthetic tests tend to show less resolution in the northern part of the rupture, this solution is compatible with the near-field data (GPS, coral heads and imagery), and would allow one to explain the apparent paradox between the large local displacements and the moderate tsunami observed locally. Finally, we demonstrate the rapidly dominating effect of propagation and slip distribution over the rupture velocity, and how it precludes the direct estimate of this latter parameter.  相似文献   
110.
We describe results of an active-source seismology experiment across the Chilean subduction zone at 38.2°S. The seismic sections clearly show the subducted Nazca plate with varying reflectivity. Below the coast the plate interface occurs at 25 km depth as the sharp lower boundary of a 2–5 km thick, highly reflective region, which we interpret as the subduction channel, that is, a zone of subducted material with a velocity gradient with respect to the upper and lower plate. Further downdip along the seismogenic coupling zone the reflectivity decreases in the area of the presumed 1960 Valdivia hypocentre. The plate interface itself can be traced further down to depths of 50–60 km below the Central Valley. We observe strong reflectivity at the plate interface as well as in the continental mantle wedge. The sections also show a segmented forearc crust in the overriding South American plate. Major features in the accretionary wedge, such as the Lanalhue fault zone, can be identified. At the eastern end of the profile a bright west-dipping reflector lies perpendicular to the plate interface and may be linked to the volcanic arc.  相似文献   
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