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金属矿产勘查技术发展现状与思考 总被引：5，自引：1，他引：5
近年来，以寻找金属矿产为目的发愤卢业的勘查新技术可概括为：（1）以寻找隐伏矿为目标的覆盖区地球物理勘查技术，其中包括“三维地震”和“高光谱遥感”技术；（2）地球化学勘查新技术，其中包括“深穿透地球化学技术”、“地球化学信息的综合解释和地球化学填图技术”；（3）“找矿信息提取和综合”技术等。限于篇幅，本文仅对地球化学勘查新技术的研究现状进行了分析，同时对下列问题进行了思考：（1）在一个地区开展地球化学找矿工作首先要确立合适的取样介质，取样介质的立应以查明成矿成晕元素的形成机制和赋存状态为基础；（2）加强不同景观条件下不同矿种和不同矿床类型的异常特征和异常模式研究，建立区分矿异常和非矿异常的模式识别模型；（3）加强不同景观地质条件下，不同勘查尺度的地球化学填图技术研究，以实现迅速掌握全局，逐步缩小靶区的找矿战略；（4）加强地球化学信息与地质、地球物理和遥感信息相结合的信息综合技术的研究，应用综合信息定量圈定和评价找矿靶区，减少矿产勘查的不确定性。 相似文献
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世界多极化和经济全球化是一种必然趋势，和平与发展虽然是主流，但我国国家安全形势不容乐观，同样面临严峻的挑战.与国家安全相关的地球物理学研究领域很广，主要涉及空间物理学、大气物理学、军事海洋学、空间遥感物理与监测和固体地球物理学.在这些领域中存在众多需要解决的问题，本文列举了一系列亟需研究的重要问题.在此基础上，笔者归纳出国家安全地球物理学的若干研究方向是：（1）具有明显或潜在国家安全应用价值的地球物理理论、方法技术研究；（2）国家安全地球物理装备（仪器）设施研究；（3）国家安全地球物理学中的数据处理理论、方法和技术研究；（4）重大国家安全地球物理学问题研究.由于国家安全地球物理学的研究任务多种多样、且各有侧重，如海、陆、空和二炮，都有各自的研究重点，不能一概而论.以二炮部队所涉及的军事地球物理学研究而论，研究方向应包括：（1）军事情报侦测保障中的地球物理问题研究（包括侦测与反侦测）；（2）作战运用与保障（测地、气象、空间天气、遥感）中的地球物理问题研究；（3）与战略导弹部队作战相关的地球物理武器和地球物理战研究；（4）国防工程中的地球物理应用研究. 相似文献
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高温高压下弹性波速测量是研究地球深部物质状态、性质和运动等问题的一种重要手段．现今人们认为，脱水是引起地球内部地震波速度异常的主要原因之一(Kern，1982；Ito，1990；Christensen，1989；Popp，Kern，1993；宋茂双等，1996；周文戈，1998；赵志丹等，1996)．地球物理、地球化学和岩石学等资料表明，云母、闪石和蛇纹石等含水矿物的脱水作用是地球深部水的主要来源(Ulmer，Tromsdorff，1995；Ito，Tatsumi，1995；Newton，1989)．蛇纹石是地幔的主要矿物——橄榄石和辉石的主要蚀变矿物，含H2O量达13%(wt)，远远高于其它含水矿… 相似文献
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地球物理信号中普遍含有噪声，消除噪声是地球物理信号处理中的关键技术之一.奇异功率谱分析（SSA）是在状态空间（又称相空间）中研究（系统）动力学、非线性科学与混沌现象的方法.本文在状态空间中通过SSA分解，研究、应用地球物理序列的尺度不变性进行多维分形滤波：通过在状态空间的SSA分解，构造了经验正交函数系（EOF）；在EOF子空间中定义了两种尺度与测度后，发现了两种测度与尺度皆在多个尺度范围内存在尺度不变性；利用这种尺度~测度的尺度不变性，设计、实现了多维分形奇异功率谱(MSSA)滤波模型；处理解释了大洋钻探（ODP）1143A孔岩芯自然反射性（NGR）资料；Fourier功率谱分析结果证明，MSSA能有效地压制噪声，提取有用信号.研究得出，嵌入维数对MSSA基本无影响（小于1/1000），多维分形滤波器（MSSA）能有效压制噪声或提取有用信号. 相似文献
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地球物理信号中普遍含有噪声，消除噪声是地球物理信号处理中的关键技术之一.奇异功率谱分析（SSA）是在状态空间（又称相空间）中研究（系统）动力学、非线性科学与混沌现象的方法.本文在状态空间中通过SSA分解，研究、应用地球物理序列的尺度不变性进行多维分形滤波：通过在状态空间的SSA分解，构造了经验正交函数系（EOF）；在EOF子空间中定义了两种尺度与测度后，发现了两种测度与尺度皆在多个尺度范围内存在尺度不变性；利用这种尺度~测度的尺度不变性，设计、实现了多维分形奇异功率谱(MSSA)滤波模型；处理解释了大洋钻探（ODP）1143A孔岩芯自然反射性（NGR）资料；Fourier功率谱分析结果证明，MSSA能有效地压制噪声，提取有用信号.研究得出，嵌入维数对MSSA基本无影响（小于1/1000），多维分形滤波器（MSSA）能有效压制噪声或提取有用信号. 相似文献
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Christian Liebske Bettina Schmickler Hidenori Terasaki Brent T. Poe Akio Suzuki Ken-ichi Funakoshi Ryota Ando David C. Rubie 《Earth and Planetary Science Letters》2005,240(3-4):589-604
The viscosity of synthetic peridotite liquid has been investigated at high pressures using in-situ falling sphere viscometry by combining a multi-anvil technique with synchrotron radiation. We used a newly designed capsule containing a small recessed reservoir outside of the hot spot of the heater, in which a viscosity marker sphere is embedded in a forsterite + enstatite mixture having a higher solidus temperature than the peridotite. This experimental setup prevents spheres from falling before a stable temperature above the liquidus is established and thus avoids difficulties in evaluating viscosities from velocities of spheres falling through a partially molten sample.
Experiments have been performed between 2.8 and 13 GPa at temperatures ranging from 2043 to 2523 K. Measured viscosities range from 0.019 (± 0.004) to 0.13 (± 0.02) Pa s. At constant temperature, viscosity increases with increasing pressure up to 8.5 GPa but then decreases between 8.5 and 13 GPa. The change in the pressure dependence of viscosity is likely associated with structural changes of the liquid that occur upon compression. By combining our results with recently published 0.1 MPa peridotite liquid viscosities [D.B. Dingwell, C. Courtial, D. Giordano, A. Nichols, Viscosity of peridotite liquid, Earth Planet. Sci. Lett. 226 (2004) 127–138.], the experimental data can be described by a non-Arrhenian, empirical Vogel-Fulcher-Tamman equation, which has been modified by adding a term to account for the observed pressure dependence of viscosity. This equation reproduces measured viscosities to within 0.08 log10-units on average. We use this model to calculate viscosities of a peridotitic magma ocean along a liquid adiabat to a depth of 400 km and discuss possible effects on viscosity at greater pressures and temperatures than experimentally investigated. 相似文献
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In a study of the origin of basalt magma, peridotite has been partially fused and the composition of the liquid phases determined. Peridotite was chosen because it is thought to be the most likely material of the upper mantle. Geological evidence suggests that the upper mantle is not of basaltic composition and eclogitic mineralogy but that it is of ultrabasic composition. Although under some conditions an ultrabasic mantle may be within the field of eclogite stability, the comparative rarity of high-pressure phases such as garnet in ultrabasic nodules suggests that normal basalts are derived from non-eclogitic regions. The peridotite composition selected for experimental work was that of average peridotite (Nockolds). Charges of the synthetic peridotite were held at constant temperature (±1/2°C) in a non-oxidising atmosphere for one week. After quenching, the glass was extracted and analysed. The glass content varied from 4% at 1250°C to 26% at 1355°C. Its composition ranged from a basalt more or less saturated in normative silica at a temperature of 1310°C (15% fusion) and below, to picrite basalt at higher temperatures. The results confirm the general assumption that basalts can be the product of the partial fusion of peridotite. To date, the experimental work has been under anhydrous conditions at atmospheric pressure. 相似文献
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Dante Canil 《Earth and Planetary Science Letters》1991,106(1-4)
Phase equilibrium experiments were performed on typical ‘oceanic’ and ‘cratonic’ peridotite compositions and a Ca, Al-rich orthopyroxene composition, to test the proposal that garnet lherzolites exsolved from high-temperature harzburgites, and to further our understanding of the origin of ancient cratonic lithospheres. ‘Oceanic’ peridotites crystallize a garnet harzburgite assemblage at pressures above 5 GPa in the temperature range 1450–1600°C, but at 5 GPa and temperatures less than 1450°C, crystallize clinopyroxene to become true lherzolites. ‘Cratonic’ peridotites crystallize a garnet harzburgite assemblage at pressures above 5 GPa in the temperature range 1300–1600°C. Garnet-free harzburgite crystallizes from both ‘cratonic’ and ‘oceanic’ peridotite at temperatures above 1450°C and pressures below 4.5–5 GPa. Phase relations for the high Ca, Al-rich orthopyroxene composition essentially mirror those for ‘oceanic’ peridotite.The complete solution of garnet and clinopyroxene into orthopyroxene observed in all three starting compositions at temperatures near or above the mantle solidus at pressures less than 6 GPa supports the hypothesis that garnet lherzolite could have exsolved from harzburgite. The inferred cooling path for the original high-temperature harzburgite protoliths of garnet lherzolites differs depending on bulk composition. The precursor harzburgite protoliths of garnet lherzolites and harzburgites with ‘cratonic’ bulk compositions apparently experienced simple isobaric cooling from formation temperatures near the peridotite solidus to those at which most of these peridotites were sampled in the mantle (< 1200°C). The cooling histories for harzburgite protoliths of sheared garnet lherzolites with ‘oceanic’ compositional affinity are speculated to have involved convective circulation of mantle material to depths deeper than those at which it was originally formed.Phase equilibria and compositional relationships for orthopyroxenes produced in phase equilibrium experiments on peridotite and komatiite are consistent with an origin for ‘cratonic’ peridotite as a residue of Archean komatiite extraction, which has since cooled and exsolved clinopyroxene and garnet to become the common low-temperature, coarse-grained peridotite thought to comprise the bulk of the mantle lithosphere beneath the Archean Kaapvaal craton. 相似文献
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Abstract Geochemical data on Baegryeong Island spinel peridotites found in Miocene alkali basalt provide the information for lithosphere composition, chemical processes, equilibrium pressure and temperature conditions. Spinel peridotite xenoliths, showing transitional textures between protogranular and porpyroclastic textures, were accidentally trapped by the ascending alkali basalt magma. The xenoliths originate at depths from 50 to 70 km with a temperature range from 800 to 1100°C. The variations of modal and mineral compositions of the spinel peridotite xenoliths indicate that the xenoliths have undergone 1–10% fractional melting. The spinel peridotites from Baegryeong Island have undergone cryptic mantle metasomatism subsequent to melt extraction. Metasomatic agent of enriched spinel peridotite xenoliths was carbonatite melt. 相似文献
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High-pressure partial melting of garnet pyroxenite: possible mafic lithologies in the source of ocean island basalts 总被引：6，自引：0，他引：6
Many ocean island basalts (OIB) that have isotopic ratios indicative of recycled crustal components in their source are silica-undersaturated and unlike silicic liquids produced from partial melting of recycled mid-ocean ridge basalt (MORB). However, experiments on a silica-deficient garnet pyroxenite, MIX1G, at 2.0-2.5 GPa show that some pyroxenite partial melts are strongly silica-undersaturated [M.M. Hirschmann et al., Geology 31 (2003) 481-484]. These low-pressure liquids are plausible parents of alkalic OIB, except that they are too aluminous. We present new partial melting experiments on MIX1G between 3.0 and 7.5 GPa. Partial melts at 5.0 GPa have low SiO2 (<48 wt%), low Al2O3 (<12 wt%) and high CaO (>12 wt%) at moderate MgO (12-16 wt%), and are more similar to primitive OIB compositions than lower-pressure liquids of MIX1G or experimental partial melts of anhydrous or carbonated peridotite. Solidus temperatures at 5.0 and 7.5 GPa are 1625 and 1825°C, respectively, which are less than 50°C cooler than the anhydrous peridotite solidus. The liquidus temperature at 5.0 GPa is 1725°C, indicating a narrow melting interval (∼100°C). These melting relations suggest that OIB magmas can be produced by partial melting of a silica-deficient pyroxenite similar to MIX1G if its melting residue contains significant garnet and lacks olivine. Such silica-deficient pyroxenites could be produced by interaction between recycled subducted oceanic crust and mantle peridotite or could be remnants of ancient oceanic lower crust or delaminated lower continental crust. If such compositions are present in plumes ascending with potential temperatures of 1550°C, they will begin to melt at about 5.0 GPa and produce appropriate partial melts. However, such hot plumes may also generate partial melts of peridotite, which could dilute the pyroxenite-derived partial melts. 相似文献
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The density distribution of the lithosphere is non-linear and discontinuous due to complex mineralogy and, most importantly, phase transitions. We evaluate the influence of changes in mantle composition on lithospheric density and its evolution during horizontal stretching, using thermodynamic calculations of the density as a function of pressure, temperature and composition. We also develop a simple parameterization based on end-member mineral reactions and geometric relationships between the geotherm and the phase boundary for comparison. The garnet–spinel peridotite transition leads to a moderate decrease in density of the mantle part of the lithospheric column at the initial stages of stretching. When the crust is sufficiently thinned and temperature is relatively high, plagioclase peridotite becomes stable in the upper part of the mantle. The density reduction due to the plagioclase-in reaction is controlled by bulk Al2O3 in the mantle and by the depth of the plagioclase-in reaction, which is mainly governed by the Na2O/Al2O3 ratio. Since Na2O and Al2O3 increase with the fertility of the mantle the phase transition effect is most pronounced for relatively fertile mantle (and strong extension) and can lead to 2.3% density reduction. This is equivalent to heating the entire lithosphere by 700 °C if only the effect of thermal expansion on density is taken into account. The formation of plagioclase peridotite can explain syn-rift uplift in sedimentary basins that experienced large mantle stretching without invoking an unrealistically strong increase in temperature. It might also be responsible for the break-up unconformity observed at continental margins. 相似文献
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为进一步探讨上地幔的高导层成因,了解碳酸盐在上地幔电性方面的作用并估算上地幔高导层的碳酸盐含量,本文对不同碳酸盐含量的橄榄岩及玄武岩样品在2~3 GPa、300~1300℃的条件下进行了电性实验研究.研究初步发现:碳酸盐熔体显著增强橄榄岩、玄武岩样品的导电能力;单纯用含硅酸盐熔体的橄榄岩或单纯用含水橄榄岩可能难以解释上地幔某些区域的异常高导现象;同样,单纯用碳酸盐化的橄榄岩可能也难以解释上地幔某些区域的高导现象;上地幔的高导区很可能是碳酸盐熔体、硅酸盐熔体及水的共存区域. 相似文献
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The connectivity of molten Fe-S in peridotite has been experimentally investigated by means of in situ electrical conductivity measurements at high temperatures and 1 GPa. Starting materials were powdered mixtures of peridotite KLB-1 with various amounts (0, 3, 6, 13, 19, 24 vol.%) of the 1 GPa eutectic composition in the Fe-FeS binary system. At temperatures above the eutectic point in the Fe-FeS system (∼980 °C) and below the solidus of KLB1 (∼1200 °C), molten Fe-S in a solid silicate matrix interconnects when the volume fraction is over ∼5%. Conductivity-temperature paths indicate that in the presence of partial silicate melting the connectivity of molten Fe-S in a peridotite matrix is inhibited. Based on observations of retrieved samples, the percolation threshold of Fe-S melts in the presence of low to moderate degrees of silicate melt is estimated at 13±2 vol.%. These results indicate that if the volume fraction of Fe-alloy in a planetesimal was initially greater than 5%, and if early heating by decay of radionuclides raised the temperature of the interior above the Fe-alloy melting point, initial metal segregation was controlled by permeable flow of molten iron alloy in a solid silicate matrix. These conditions were likely met by many terrestrial objects in the early solar nebula. Efficient removal of residual Fe-alloy (5 vol.%) from silicate requires high-degree melting of silicate so that metal can segregate as droplets. Giant impacts during the final stage of accretion of large planetary objects could supply the energy required for high-degrees of melting. Alternatively, if initial metal segregation were delayed until a planetary object grew to large size (∼1000 km in diameter), release of gravitational potential energy due to metal segregation could contribute enough heat to form a magma ocean. 相似文献
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Melting experiments on a high-magnesian andesite 总被引：1，自引：0，他引：1
Yoshiyuki Tatsumi 《Earth and Planetary Science Letters》1981,54(2):357-365
Melting experiments were conducted on a high-magnesian bronzite olivine andesite (Teraga-Ike andesite) which is considered to be a primary andesite. The high-magnesian andesite magma is in equilibrium with both olivine and orthopyroxene at about 15.5 kbar and 1080°C under H2O-saturated conditions and at lower pressure and higher temperature under H2O-undersaturated conditions. This suggests that high-magnesian andesites could be generated by the partial melting of upper mantle peridotite containing a small amount of H2O. 相似文献