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1.
M.J. Drury 《Physics of the Earth and Planetary Interiors》1978,17(2):P16-P20
Modelled conductivity variations with depth in the upper mantle obtained from geomagnetic induction and magnetotelluric results are compared to predicted conductivity variations obtained from laboratory measurements on dry material assumed to occur in the mantle. Higher than predicted conductivities at the base of the oceanic lithosphere suggest the presence of highly conductive partial melt. Using a known relationship between observed conductivity and the conductivity and volume fraction of the fluid, estimates of the melt volume fraction have been made assuming the melt to be in continuously connected network. In the sub-oceanic asthenosphere these values range from approximately 0.45 to 9%, whereas in sub-continental asthenosphere the partial melt volume fraction appears to be too low to increase the bulk conductivity. The partial melt content of the sub-continental asthenosphere may reach a few percent if the melt exists in isolated pockets. The apparent difference in melt content in sub-oceanic and sub-continental asthenosphere is discussed in terms of the different velocities of Pacific-type plates (which carry no continental block) and Atlantic-type plates (which carry a continental block). 相似文献
2.
CRYSTALLOGRAPHIC PREFERRED ORIENTATION(CPO) OF ANISOTROPIC MINERALS IN THE LITHOSPHERE AND ITS SIGNIFICANCE TO THE STUDY OFLITHOSPHERE DYNAMICS 
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下载免费PDF全文 Seismic anisotropy has been widely used to constrain deformation and mantle flow within the upper mantle of the Earth's interior, and is mainly affected by crystallographic preferred orientation(CPO)of anisotropic mineral in lithosphere. Anisotropy of peridotites caused by deformation is the main source of seismic anisotropy in the upper mantle. Olivine is the most abundant and easily deformed mineral to form CPO in peridotite, thus the CPO of olivine controls seismic anisotropy in the upper mantle. Based on simple shear experiments and studies of natural peridotites deformation, several CPO types of olivine have been identified, including A, B, C, D, E and AG-type. Studies on the deformation of olivine have shown that the CPO of olivine is mainly related to stress, water content, temperature, pressure, partial melting and melt/fluid percolation. Most of the seismic anisotropy has been explained by the A-type olivine CPO in the upper mantle, which is commonly found in upper-mantle peridotites and produced by the simple shear in dry conditions. Previous studies showed that anisotropy was attributed to the CPO of mica and amphibole in the middle-lower crust. The comparison between mantle anisotropy calculated from mineral CPO and regional anisotropy deduced from geophysical methods is therefore particularly useful for interpreting the deformation mechanisms and geodynamic processes which affect the upper mantle in different tectonic units such as subduction system, continental rift and continental collision zone in the world. The paper summarizes the characteristics of CPO and anisotropy of major anisotropic minerals in the upper mantle. Taking the lithosphere mantle xenoliths in the southeastern Tibetan plateau as an example, we perform detailed studies on the microstructures and seismic anisotropy to better understand the deformation mechanisms and upper mantle anisotropy in this region. Results show that the CPO of olivine in peridotite xenoliths in southeastern Tibetan plateau are A-type and AG-type. The mechanisms proposed for the formation of AG-type are different from that for the A-type. Therefore, the occurrence of AG-type olivine CPO pattern suggests that this CPO may record a change in deformation mechanism and tectonic environment of the lithosphere in southeastern Tibetan plateau. Provided that the strong SKS(shear wave splitting)observed in southeastern Tibetan plateau results from lithosphere mantle, the lithosphere mantle in this region is expected to be at least 130km thick and characterized by vertical foliation. Considering that the thickness of lithosphere in southeastern Tibetan plateau is much less than 130km and the lithosphere mantle cannot explain the anisotropy measured by SKS, other anisotropy sources should be considered, such as anisotropy in the asthenosphere and the oriented melt pockets(MPO)in the upper mantle. Therefore, detailed study of CPO of anisotropic mineral is essential for constraining geophysical measurements and analyzing the dynamic process of the lithosphere reasonably. 相似文献
3.
目前存在有多种地幔热导率模型,不同模型在数值和随温压变化的特征上有明显的差异.为探究不同热导率模型对动力学数值模拟结果的影响,本文对不同模型下的岩石圈张裂过程进行模拟研究,探讨地幔热导率对岩石圈热传输、变形和熔融过程的影响及其作用机理.结果显示,不同热导率模型下,岩石圈的变形和熔融特征表现出明显差异.高热导率模型下,岩石圈破裂较晚,形成陆缘较为宽阔,地壳熔融强烈而地幔熔融较弱;低热导率模型下,岩石圈破裂较早,形成陆缘较为狭窄,地幔熔融强烈而地壳熔融较弱.这种差异源于不同地幔热导率下岩石圈和地幔热状态的变化及相应力学性质的改变.高热导率下,热传导的增温效应显著,岩石圈呈现较热的状态,其强度整体较低,壳幔耦合减弱;而低热导率下,热对流的增温效应显著,岩石圈呈较冷的状态,其强度整体较高,壳幔耦合增强.基于模拟结果,本文认为地幔热导率的选取对动力学模拟的结果有着较为显著的影响,相对于随温压的变化,热导率数值的差异对动力学数值模拟的结果影响更大,尤其是对于地幔熔融过程的影响. 相似文献
4.
Kiyoshi Baba 《Surveys in Geophysics》2005,26(6):701-731
This review paper presents recent research on electrical conductivity structure in various marine tectonic settings. In at
least three areas, marine electromagnetic studies for structural exploration have increasingly progressed: (1) data accumulations,
(2) technical advances both for hardware and software, and (3) interpretations based on multidisciplinary approaches. The
mid-ocean ridge system is the best-studied tectonic setting. Recent works have revealed evidence of conductive zones of hydrothermal
circulation and axial magma chambers in the crust and partial melt zones of the mid-ocean ridge basalt source in the mantle.
The role of water or dissolved hydrogen and its redistribution at mid-ocean ridges is emphasized for the conductivity pattern
of the oceanic lithosphere and asthenosphere. Regions of mantle upwelling (hotspot or plume) and downwelling (subducting slab)
are attracting attention. Evidence of heterogeneity exists not only in the crust and the upper mantle, but also in the mantle
transition zone. Electrical conductive zones frequently overlap seismic low-velocity zones, but discrepancies are also apparent.
Some studies have compared conductivity models with the results of seismic and other studies to investigate the physical properties
or processes. A new laboratory-based conductivity model for matured oceanic lithosphere and asthenosphere is proposed. It
takes account of both the water distribution in the mantle as well as the thermal structure. It explains observed conductivity
patterns in the depth range of 60–200 km. 相似文献
5.
Magnetotelluric (MT) studies represent the structure of crust and mantle in terms of conductivity anomalies, while geodynamic modelling predicts the deformation and evolution of crust and mantle subject to plate tectonic processes. Here, we review the first attempts to link MT models with geodynamic models. An integration of MT with geodynamic modelling requires the use of relationships between conductivity and rheological parameters such as viscosity and melt fraction, which are provided by laboratory measurements of rock properties. Owing to present limitations in our understanding of these relationships, and in interpreting the trade-off between scale and magnitude of conductivity anomalies from MT inversions, most studies linking MT and geodynamic models are qualitative rather than providing hard constraints. Some recent examples attempt a more quantitative comparison, such as a study from the Himalayan continental collision zone, where rheological parameters have been calculated from a resistivity model and compared to predictions from geodynamic modelling. We conclude by demonstrating the potential in combining MT results and geodynamic modelling with examples that directly use MT results as constraints within geodynamic models of ore bodies and studies of an active volcano-tectonic rift. 相似文献
6.
通过地质、地球物理和地球化学资料分析,建立了东秦岭地学断面带地壳二维深度-强度剖面,揭示了该造山带的地壳结构和流变学分层性．脆性的上地壳南薄北厚;中、下地壳包括莫霍面呈现水平流变状态,南端蠕变特征更明显;上地幔流变强度较大其地壳类型是栾川以南为H型地壳,构成中、新生代造山带的核部,具有伸展构造和走滑构造的特征,栾川以北为C型地壳,中、新生代的大陆汇聚带．东秦岭地学断面带整体上看为C-H型地壳,反映了后造山期陆内造山的构造特征．地壳物质为长英质-石英闪长质壳内软层具有低速、高热、强网状反射和低强度蠕变的地球物理特征,是后造山期经过调整的水平流变层. 相似文献
7.
以中国大陆西北地区地震层析成像的结果为基础，通过分析大陆块体内部岩石层和软流层的深部形态，提出西部造山带与相邻块体之间几种可能的碰撞类型：天山与塔里木之间存在地块的嵌入拼合、俯冲、岩石层拆离下沉以及层间插入等多种构造样式；青藏高原与北部地质单元之间存在十分清晰的深部边界，反映出上地幔物质向北扩展的痕迹；推测青藏高原的岩石层在向北运动的过程中由于受到塔里木刚性块体的阻滞发生弯曲甚至折断，但是祁连山以北较浅的软流层相当于一个开放边界，使高原的上地幔物质得以进一步向北迁移.大陆碰撞不仅造成中国西部造山带岩石层结构的变动，而且导致软流层中一部分熔融的岩浆体沿着碰撞边界上涌到岩石层底部，它们对青藏高原以及西部造山带的形成演化起到重要的作用. 相似文献
8.
本文利用重力数据采用Parker-Oldenburg方法反演了南北构造带及邻域地区的地壳厚度,同时采用体波地震层析成像方法反演了研究区的地壳至上地幔的三维速度结构.根据计算结果对研究区的地壳及岩石层结构进行了探讨,力图揭示南北构造带及邻域地壳、岩石层变形特征,并且对青藏高原边缘活动带壳幔构造演化的深部成因、研究区的上地幔流变性及其动力学意义进行了相应的讨论.通过分析研究表明南北构造带地区为地壳厚度剧变区,西侧为地壳增厚区,东侧的鄂尔多斯、四川盆地为地壳稳定区,而再向东为地壳逐渐减薄区.中国岩石层减薄与增厚的边界基本被限定在大兴安岭—太行山—秦岭—大巴山—武陵山一带,这也是东部陆缘带和中部扬子、鄂尔多斯克拉通地区深部构造边界的分界线,其两侧不仅浅层地质构造存在较大的差异,上地幔深部的物性状态和热活动也明显不同,这说明研究区的岩石层和软流层结构以及深部物质的分布存在横向非均匀性.中部地区和青藏高原深部构造边界的分界线位于东经100°—102°左右. 相似文献
9.
10.
本文首先论述了板块学说提出的过程和存在的一些不足与疑问,特别是该学说将Holmes（1948）的地幔热对流说作为驱使岩石圈板块运动的动力机制.而后又以青藏高原及邻区为例,根据区域地质、蛇绿岩和地质构造研究的成果,特别是地震测深研究的成果,详细地论证了本区不存在有大洋中脊扩张成为大洋盆地的新大洋和大洋板块简单的B型俯冲模式,但存在有海底扩张的陆间海和海洋地壳板片（蛇绿岩构造岩片）的仰冲以及大陆岩石圈板片复杂的A型俯冲新模式.新模式不是以地幔对流运动,而是以扩张分离A型俯冲的大陆岩石圈板片与软流圈之间的水平剪切相对运动机制作为它的躯动力. 相似文献
11.
A. Ádám 《Surveys in Geophysics》1980,4(1-2):43-55
Magnetotelluric soundings show that the conductivity increases in the asthenosphere. The depth of this conductivity zone decreases with an increase of the surface heat flow, i.e. in such cases the lithospheric plate is thinner. The depth of the velocity decrease of seismic shear wave (S waves) shows the same connection with the surface heat flow. The solidus of a mixed-volatile medium intersects the temperature curves belonging to different surface heat flows at depths where the conductivity increase and the velocity decrease appear. These connections point to partial melting in the asthenosphere, which can decrease the viscosity too, and help the movement of the lithospheric plates according to the ideas of global tectonics.The melt fraction of peridotite and pyrolite determined by Shankland and Waff from the effective conductivity of the asthenosphere is about 3–4% at 30 kbar and ato
*=0.1 S m–1.In the upper mantle of old shields it is likely that there is no well-developed asthenosphere due to the low temperature. Over these so-called viscous anchors the lithospheric plates do not move. It is supposed that the conductivity increases observed below crystalline shields at a depth of about 300 km indicate the phase transition of rocks. Thus in these areas the surface of the phase transition can be at a higher position than in the younger tectonic units. 相似文献
12.
Auke Barnhoorn Martyn R. Drury Herman L.M. van Roermund 《Earth and Planetary Science Letters》2010,289(1-2):54-67
The rheological properties of upper mantle rocks play an important role in controlling the dynamics of the lithosphere and mantle convection. Experimental studies and microstructures in naturally deformed mantle rocks usually imply that olivine controls the upper mantle rheology. Here we show for the first time evidence from the geometry of folded compositional layers in mantle rocks from Western Norway that garnet-rich rocks can have lower solid-state viscosities than olivine-rich rocks. Modeling of melt-free and dry rheology of garnet and olivine confirms that the reversed viscosity contrast between garnet-rich and olivine-rich layers for this folding event can be achieved over a relatively wide range of temperatures at low stress conditions when the fine-grained garnet deforms by diffusion creep while the coarse-grained olivine deforms by dislocation creep and/or diffusion creep.In general, modeling of the fold viscosity contrast shows that in the stable subcontinental lithospheric mantle or convecting mantle such a reversed viscosity contrast can be formed due to diffusion creep processes in fine-grained garnets in a dry mantle environment or at conditions where the garnet-pyroxene layer is partially molten, i.e. close to solidus–liquidus conditions in the upper mantle. Alternatively in cold plate tectonic settings, e.g. in subduction zones, some water-weakening is a feasible mechanism to create the reversed viscosity contrast between garnet and olivine. 相似文献
13.
M.J. Bickle 《Earth and Planetary Science Letters》1986,80(3-4):314-324
The increased depth and volume of melting induced in a higher temperature Archaean mantle controls the stability of the lithosphere, heat loss rates and the thickness of the oceanic crust. The relationship between density distributions in oceanic lithosphere and the depth of melting at spreading centres is investigated by calculating the mineral proportions and densities of residual mantle depleted by extraction of melt fractions. The density changes related to compositional gradients are comparable to those produced by thermal effects for lithosphere formed from a mantle which is 200°C or more hotter than modern upper mantle. If Archaean continental crust formed initially above oceanic lithosphere, the compositional density gradients may be sufficient to preserve a thick Archaean continental lithosphere within which the Archaean age diamonds are preserved. The amount of heat advected by melts at mid-ocean ridges today is small but heat advected by melting becomes proportionally more important as higher mantle temperatures lead to a greater volume of melt and as the rate of production of oceanic plates increases. Archaean tectonics could have been dominated by spreading rates 2–3 times greater than now and with mantle temperatures between ca. 1600°C and 1800°C at the depth of the solidus. Mid-ocean ridge melting would produce a relatively thick but light refractory lithosphere on which continents could form, protected from copious volcanism and high mantle temperatures. 相似文献
14.
D.C. Tozer 《Physics of the Earth and Planetary Interiors》1981,25(3):280-296
An adequate theory of continental drift can be based on heat transfer theory, but it does demand the acceptance of a large downward revision of traditional estimates of average upper mantle temperatures and a consistent understanding of lithosphere and asthenosphere in terms of a difference in rheological behaviour under prolonged non-hydrostatic stress. The recognition that an extremely viscous average state of the upper mantle is self regulating both requires and permits an explanation of magma generation at a strictly limited rate (when averaged for the whole planet over a few years) in terms of unsteady and local deformational heating.The activity of water as a reducer of silicate creep resistance is used to develop the hypothesis that water produced by an amphibole dehydration has been effectively trapped in the Earth and is the underlying cause of a low seismic Q ～ 50 and an electrical conductivity 10?2 ?10?1 ohm?1 m?1, at depths of ～ 100 km. At the predicted low horizontally-avera temperatures, the conductivity contrast of rock and aqueous solutions is very large, and mantle electrical conductivity studies now look best-suited to explore this trapping process, and the distinctly recognisable possibility that the uptake of ocean water in the subduction process exceeds the rate of loss that can be explained purely through magmatic activity. 相似文献
15.
岩石圈-软流圈边界(lithosphere-asthenosphere boundary)是上地幔内具有负速度梯度的地震波速度界面.对俯冲带区域LAB开展地震学探测有助于进一步认识岩石圈和软流圈的相互作用以及与板块俯冲有关的地球动力学过程.本文收集了2006-2012年发生于南美中部地区4个深源地震的垂向宽频带波形资料,利用线性倾斜叠加处理得到了相对走时-慢度域的灰度图,并成功提取了sP在LAB底反射的前驱震相S_(LAB)P.基于改进的一维速度模型IASP91-SA计算得出了6个S_(LAB)P震相反射点的水平分布,并划分为西部(Ⅰ)和东部(Ⅱ)分区:分区工内LAB深度位于60~63 km,平均深度为61 km,起伏为3 km;分区Ⅱ内LAB深度位于78~82 km,平均深度为80 km,起伏为4 km.研究结果显示南美中部地区LAB深度自西向东呈变大的趋势,这可能反映了大陆岩石圈受改造程度的差异.我们推测在靠近海沟的地区,软流圈内部分熔融程度较高且熔体较为富集,对大陆岩石圈的侵蚀作用较强;在远离海沟的地区,软流圈内部分熔融程度降低且熔体分布减少,对大陆岩石圈的侵蚀作用减弱. 相似文献
16.
According to a large volume of data an intensive crustal uplift began in the Oligocene over most of the continental areas after a long period of relative tectonic stability. This Neotectonic uplift formed most of the present positive topographic features on the continents, and its strong acceleration took place during the last several million years. In many regions the uplift was associated with magmatism. The main methods of studying the Neotectonic uplift are considered together with the data on the uplift of Southern Africa. In this area the uplift took place in the Early Miocene (up to 300 m) and in the Late Pliocene and Pleistocene (up to 900 m). It occurred without stretching or shortening of the crust. Rapid erosion of the lower part of mantle lithosphere by a plume material is proposed as a mechanism of the uplift. This material ascended from below and rapidly spread along the base of the lithosphere. Its spreading for 1000 km during a few million years is possible only under a low viscosity of normal asthenosphere (1019 Pa s) and a much lower viscosity of a plume material (2 × 1016 Pa s). As in Southern Africa, in most of the regions the Neotectonic uplift was associated with insignificant shortening or stretching of the crust. This indicates that in some regions a plume material ascended from below and rapidly spread along the base of the lithosphere and eroded the mantle lithosphere in vast areas beneath the continents. In regions with a hot asthenosphere a strong weakening of the mantle lithosphere which allows its erosion can be associated with a high temperature of the plume material. In regions where the asthenosphere is at moderate temperature weakening of the mantle lithosphere can result from infiltration of volatiles from the plume material. 相似文献
17.
A. P. Trubitsyn 《Izvestiya Physics of the Solid Earth》2013,49(5):668-674
The formation of the thermal cross section of the lithosphere and mantle upon the interaction between the mantle convection and the immobile continent surrounded by the oceanic lithosphere is studied by numerical modeling. The convective temperature and velocity fields and then the averaged geotherms for subcontinental and suboceanic regions up to the boundary with the core are calculated from the solution of convection equations with a jump in viscosity in the continental zone. Using the experimental data on the solidus temperature in the rocks of the upper mantle, the average thickness of the continental and oceanic lithosphere is estimated at 190 and 30 km, respectively. The effect of a hot spot formed in the subcontinental upper mantle at a depth of 250–500 km, which has not been previously noted, is revealed. Although the temperature in this zone is typically assumed to be close to adiabatic, the calculations show that it is actually higher than adiabatic by up to 200°C. The physical mechanism responsible for this effect is associated with the accumulation of convective heat beneath the thermally insulating layer of the continental lithosphere. The revealed anomalies can be important in studying the phase and mineral transformations at the base of the lithosphere and in the regional geodynamical reconstructions. 相似文献
18.
松辽盆地作为东亚裂谷系的一部分，与华北克拉通一起经历了中生代岩石圈减薄的重大地质事件.对大陆岩石圈-软流圈状态和构造的整体认识，是研究大陆岩石圈减薄深部动力学过程的关键.在获得过松辽盆地的106个宽频和30个长周期大地电磁测深数据的基础上，完成测点数据二维偏离度、构造走向等计算与分析，进一步采用非线性共轭梯度算法，对TE和TM模式数据进行二维联合反演，获得了沿剖面的壳-幔电性结构，并依此构建了松辽盆地壳-幔结构模型.研究结果表明：（1）大兴安岭地区岩石圈厚度约为160 km，松辽盆地岩石圈厚度约为45 km，张广才岭岩石圈厚度在70~100 km之间，莫霍面与岩石圈底界面不呈镜像关系.软流圈整体表现为中、低阻异常，电阻率值在30 Ωm左右，其形态呈西倾约30°的蘑菇状异常，指示了软流圈物质上涌的形式，有别于软流圈垂直上涌的传统认识.（2）松辽盆地深部存在双层高导异常（电阻率小于5 Ωm），上层为壳内高导层，呈"蛇"状分布，推断为岩浆底侵区，下层为幔内高导层，呈"哑铃"状，为软流圈上涌区.软流圈内存在两个"哑铃"状中、高阻异常，推断为拆沉的岩石圈地幔.具有冷的、高密度的下降物质流的堆积以及拆沉块体下插到两侧山岭是促使大兴安岭与张广才岭在中生代伸展环境中快速隆升重要原因；（3）松辽盆地经历了岩石圈减薄事件，与大兴安岭岩石圈厚度相比，松辽盆地岩石圈厚度减薄了近100 km，与东侧张广才岭相比减薄了70 km，而与中生代华北地台100 km的岩石圈厚度相比，减薄了近50 km，其经历了岩石圈伸展期、裂解期、拆沉期和增长期的动力学过程. 相似文献
19.
Kerrich Robert Goldfarb Richard Groves David Garwin Steven Jia Yiefei 《中国科学:地球科学(英文版)》2000,43(1):1-68
There are six distinct classes of gold deposits, each represented by metallogenic provinces, having 100's to >1000 tonne gold production. The deposit classes are: (1) orogenic gold; (2) Carlin and Carlin-like gold deposits; (3) epithermal gold-silver deposits; (4) copper-gold porphyry deposits; (5) iron-oxide copper-gold deposits; and (6) gold-rich volcanic hosted massive sulfide (VMS) to sedimentary exhalative (SEDEX) deposits. This classification is based on ore and alteration mineral assemblages; ore and alteration metal budgets; ore fluid pressure(s) and compositions; crustal depth or depth ranges of formation; relationship to structures and/or magmatic intrusions at a variety of scales; and relationship to the P-T-t evolution of the host terrane. These classes reflect distinct geodynamic settings. Orogenic gold deposits are generated at mid-crustal (4–16 km) levels proximal to terrane boundaries, in transpressional subduction-accretion complexes of Cordilleran style orogenic belts; other orogenic gold provinces form inboard, by delamination of mantle lithosphere, or plume impingement. Carlin and Carlin-like gold deposits develop at shallow crustal levels (<4 km) in extensional convergent margin continental arcs or back arcs; some provinces may involve asthenosphere plume impingement on the base of the lithosphere. Epithermal gold and copper-gold porphyry deposits are sited at shallow crustal levels in continental margin or intraoceanic arcs. Iron oxide copper-gold deposits form at mid to shallow crustal levels; they are associated with extensional intracratonic anorogenic magmatism. Proterozoic examples are sited at the transition from thick refractory Archean mantle lithosphere to thinner Proterozoic mantle lithosphere. Gold-rich VMS deposits are hydrothermal accumulations on or near the seafloor in continental or intraoceanic back arcs.
The compressional tectonics of orogenic gold deposits is generated by terrane accretion; high heat flow stems from crustal thickening, delamination of overthickened mantle lithosphere inducing advection of hot asthenosphere, or asthenosphere plume impingement. Ore fluids advect at lithostatic pressures. The extensional settings of Carlin, epithermal, and copper-gold porphyry deposits result from slab rollback driven by negative buoyancy of the subducting plate, and associated induced convection in asthenosphere below the over-riding lithospheric plate. Extension thins the lithosphere, advecting asthenosphere heat, promotes advection of mantle lithosphere and crustal magmas to shallow crustal levels, and enhances hydraulic conductivity. Siting of some copper-gold porphyry deposits is controlled by arc parallel or orthogonal structures that in turn reflect deflections or windows in the slab. Ore fluids in Carlin and epithermal deposits were at near hydrostatic pressures, with unconstrained magmatic fluid input, whereas ore fluids generating porphyry copper-gold deposits were initially magmatic and lithostatic, evolving to hydrostatic pressures. Fertilization of previously depleted sub-arc mantle lithosphere by fluids or melts from the subducting plate, or incompatible element enriched asthenosphere plumes, is likely a factor in generation of these gold deposits. Iron oxide copper-gold deposits involve prior fertilization of Archean mantle lithosphere by incompatible element enriched asthenospheric plume liquids, and subsequent intracontinental anorogenic magmatism driven by decompressional extension from far-field plate forces. Halogen rich mantle lithosphere and crustal magmas likely are the causative intrusions for the deposits, with a deep crustal proximal to shallow crustal distal association. Gold-rich VMS deposits develop in extensional geodynamic settings, where thinned lithosphere extension drives high heat flow and enhanced hydraulic conductivity, as for epithermal deposits. Ore fluids induced hydrostatic convection of modified seawater, with unconstrained magmatic input. Some gold-rich VMS deposits with an epithermal metal budget may be submarine counterparts of terrestrial epithermal gold deposits. Real time analogs for all of these gold deposit classes are known in the geodynamic settings described, excepting iron oxide copper-gold deposits.
相似文献20.
Giacomo Corti Marco Bonini Fabrizio Innocenti Piero Manetti Giovanni B. Piccardo Giorgio Ranalli 《Journal of Geodynamics》2007,43(4-5):465-483
Analogue models are used to investigate extension of a continental lithosphere weakened by asthenospheric melts percolating through the upper mantle, a process that has been hypothesised to control the opening of the Ligurian Tethys. Models were performed in a centrifuge apparatus and reproduced, by using materials such as sand and viscous mixtures, extension of 60-km thick, three-layer continental lithosphere floating above the asthenosphere. The percolated lithospheric mantle was assumed to be characterised by a rheological behaviour similar to that of the asthenosphere. Two sets of experiments investigated the influence on deformation of (1) the thickness of the percolated mantle and the associated strength contrast between the normal and weakened lithosphere, and (2) the lateral width of the weakened zone. Model results suggest that mantle percolation by asthenospheric melts is able to promote strong localised thinning of the continental lithosphere, provided that a significant thickness of the lithospheric mantle is weakened by migrating melts within a narrow region. Strain localisation is maximised for percolation of the whole lithospheric mantle and strong strength contrast between the normal and weakened lithosphere. Under these conditions, the thickness of the lithosphere may be reduced to less than 12 km in 3 Ma of extension. Conversely, localised thinning is strongly reduced if the thickness of the percolated zone is ≤1/3 of the thickness of the whole lithospheric mantle and/or the lithosphere is weakened over wide regions. Overall, model results support the working hypothesis that mantle percolation by asthenospheric melts is a controlling factor in the transition from distributed continental deformation to localised oceanic spreading. 相似文献