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991.
桃花-石门金矿带位于秦岭地槽区北秦岭纬向褶皱带的北端黑沟和瓦穴子断裂所夹持的前加里东褶皱带中。矿床类型为石英脉型,石英脉规模小,数量多,分布于瓦穴子断裂北侧。矿脉的产出受地层、构造控制、成矿与岩性、构造、岩浆活动,温度等关系密切。  相似文献   
992.
本文用长周期763地震仪面波群速度资料反演了中国南北带及邻区的三维速度结构.其中采集238条瑞利波和358条勒夫波混合频散曲线,使用均等显示滤波方法,并以4°×4°为一格将我国境内分为147格.用随机逆反演方法得到了研究区16格的纯路径频散.面波速度结构及演结果表明:1.莫霍界面深度一般在40-50km之间,最深达65km.总趋势是从东到西加深,且在南北带西侧南北两端向中部明显加深,东侧变化小.2.地幔顶部普遍出现很厚的低速层,上界面一般埋深60-80km.上地幔顶盖厚度一般为20-60km,速度为4.30-4.50km/s.3.研究区普遍存在各向异性,而且勒夫波和瑞利波速度的差值(VSV-VSH)的绝对值随深度有增大的特点,在南北带南部和西北部VSV-VSH各向异性现象更为明显.  相似文献   
993.
造山带构造研究中几个重要学术概念问题的讨论   总被引:1,自引:0,他引:1  
张长厚  吴正文 《地质论评》2002,48(4):337-344
简要分析和评述了造山带构造研究中的几个重要学术概念问题:造山带,造山带类型、造山作用和造山过程、造山带构造格局、造山作用模式。指出不宜将造山带定义直接与板块边缘构造位置和板块间相互作用联系在一起;造山作用和造山带不仅出现在板块之间相互作用的地带,而且可以出现在远离板边界的地方--即所谓板内造山带。强调了板内造山带研究的重要性,提出了确定板内造山的主要依据,指出在造山带分类、造山带构造山带。强调了板内造山带研究的重要性,提出了确定内造山带的主要依据,指出在造山带分类、造山带构造格局和造山作用过程中应充分注意内造山带的客观存在,以及板内造山带成因动力机制研究中需要着重考虑的重要方面。  相似文献   
994.
李巍 《地质与资源》2015,24(6):554-559,576
凌源-阜新金矿成矿带是辽西及辽宁省至关重要的金成矿带.区内出露的各时代地层较齐全,与成矿关系最密切的为建平群小塔子沟组.构造运动发育从太古宙到中生代均有较大规模的构造活动,同时这些构造运动也控制了岩浆岩的侵入和金矿的形成与分布.成矿带内发育含金石英脉型金矿和次火山热液型金矿两种类型的金矿.通过对区域地质背景、典型矿床特征分析,总结了凌源-阜新金成矿带的金矿的赋矿层位、构造对金矿的控制作用及侵入岩与金矿的时空关系等3个方面的找矿标志.  相似文献   
995.
The West Junggar Orogenic Belt(WJOB)in northwestern Xinjiang,China,is located in the core of the western part of the Central Asian Orogenic Belt(CAOB).It has suffered two stage tectonic evolutions in Phanerozoic,before and after the ocean–continental conversion in Late Paleozoic.The later on intracontinental deformation,characterized by the development of the NE-trending West Junggar sinistral strike-slip fault system(WJFS)since Late Carboniferous and Early Permian,and the NW-trending Chingiz-Junggar dextral strike-slip fault(CJF)in Mesozoic and Cenozoic,has an important significance for the tectonic evolution of the WJOB and the CAOB.In this paper,we conduct geometric and kinematic analyses of the WJOB,based on field geological survey and structural interpretation of remote sensing image data.Using some piercing points such as truncated plutons and anticlines,an average magnitude of^73 km for the left-lateral strike-slip is calculated for the Darabut Fault,a major fault of the WJFS.Some partial of the displacement should be accommodated by strike-slip fault-related folds developed during the strike-slip faulting.Circular and curved faults,asymmetrical folds,and irregular contribution of ultramafic bodies,implies potential opposite vertical rotation of the Miao’ergou and the Akebasitao batholiths,resulted from the sinistral strike-slipping along the Darabut Fault.Due to conjugate shearing set of the sinistral WJFS and the dextral CJF since Early Mesozoic,superimposed folds formed with N–S convergence in southwestern part of the WJOB.  相似文献   
996.
松潘造山带马尔康强过铝质花岗岩的成因及其构造意义   总被引:2,自引:0,他引:2  
松潘造山带广泛出露印支期后碰撞型花岗岩类, 其中包括埃达克质花岗岩类、A型花岗岩和I型花岗岩, 但目前人们对该区印支期强过铝质花岗岩尚未有深入的研究.松潘造山带马尔康花岗岩属于强过铝质花岗岩(A/CNK=1.10~1.20), 其岩石类型主要为中粒二云母花岗岩和中细粒二云母花岗岩.利用LA-ICP-MS锆石U-Pb定年方法, 获得中粒二云母花岗岩的岩浆结晶年龄为208±2Ma, 中细粒二云母花岗岩的岩浆结晶年龄为200±2Ma.马尔康强过铝质花岗岩K2O/Na2O=1.13~1.75, 富Rb、Th和U, 贫Sr、Ba、Co和Ni等元素; 稀土元素组成上显示存在强到中等的负Eu异常(Eu/Eu*=0.15~0.65);全岩初始87Sr/86Sr比值(ISr) 为0.70712~0.71137, εNd (t) =-10.36~-8.43, 锆石εHf (t) =-11.8~-1.1.地球化学和Sr-Nd-Hf同位素组成一致表明, 它们的岩浆来自于地壳物质的部分熔融, 其中中粒二云母花岗岩的源岩类型主要为地壳中的泥质岩类, 而中细粒二云母花岗岩的源岩主要为地壳中的杂砂岩类.结合松潘带的地质背景、区域构造-岩浆事件及其岩浆岩的组合分析, 印支期岩石圈拆沉作用可以用来解释马尔康强过铝质花岗岩的形成机制.在松潘带, 印支期岩石圈拆沉作用导致软流圈物质上涌, 这不仅促使了加厚下地壳物质发生部分熔融, 如松潘带印支期埃达克质和I型花岗岩浆的形成, 而且还诱发了中地壳物质的部分熔融, 如马尔康强过铝质花岗岩的形成.这表明松潘带印支期岩石圈拆沉作用已使地壳不同层次发生部分熔融作用.   相似文献   
997.
According to climate features and river runoff conditions, Xinjiang could be divided into three research areas: The Altay-Tacheng region, the Tianshan Mountain region and the northern slope of the Kunlun Mountains. Utilizing daily observations from 12 sounding stations and the annual runoff dataset from 34 hydrographical stations in Xinjiang for the period 1960-2002, the variance of the summertime 0℃ level height and the changing trends of river runoff are analyzed both qualitatively and quantitatively, through trend contrast of curves processed by a 5-point smoothing procedure and linear correlation. The variance of the summertime 0℃ level height in Xinjiang correlates well with that of the annual river runoff,especially since the early 1990s, but it differs from region to region, with both the average height of the 0℃ level and runoff quantity significantly increasing over time in the Altay-Tacheng and Tianshan Mountain regions but decreasing on the northern slope of the Kunlun Mountains. The correlation holds for the whole of Xinjiang as well as the three individual regions, with a 0.01 significance level. This indicates that in recent years, climate change in Xinjiang has affected not only the surface layer but also the upper levels of the atmosphere, and this raising and lowering of the summertime 0℃ level has a direct impact on the warming and wetting process in Xinjiang and the amount of river runoff. Warming due to climate change increases the height of the 0℃ level, but also speeds up, ice-snow melting in mountain regions, which in turn increases river runoff, leading to a season of plentiful water instead of the more normal low flow period.  相似文献   
998.
By examining the absolute magnitude (H) distributions (hereafter HD) of the cold and hot populations in the Kuiper belt and of the Trojans of Jupiter, we find evidence that the Trojans have been captured from the outer part of the primordial trans-neptunian planetesimal disk. We develop a sketch model of the HDs in the inner and outer parts of the disk that is consistent with the observed distributions and with the dynamical evolution scenario known as the ‘Nice model’. This leads us to predict that the HD of the hot population should have the same slope of the HD of the cold population for 6.5<H<9, both as steep as the slope of the Trojans' HD. Current data partially support this prediction, but future observations are needed to clarify this issue. Because the HD of the Trojans rolls over at H∼9 to a collisional equilibrium slope that should have been acquired when the Trojans were still embedded in the primordial trans-neptunian disk, our model implies that the same roll-over should characterize the HDs of the Kuiper belt populations, in agreement with the results of Bernstein et al. [Bernstein, G.M., and 5 colleagues, 2004. Astron. J. 128, 1364-1390] and Fuentes and Holman [Fuentes, C.I., Holman, M.J., 2008. Astron. J. 136, 83-97]. Finally, we show that the constraint on the total mass of the primordial trans-neptunian disk imposed by the Nice model implies that it is unlikely that the cold population formed beyond 35 AU.  相似文献   
999.
随着现代工业的发展,城市黑臭河道问题日趋严重,严重影响了城市形象、生态环境和居民身心健康。利用多水塘活水链人工湿地技术净化江苏常州永胜河河水水质。监测结果显示:该技术使水体总氮浓度削减了92.0%、总磷浓度削减了82.9%,处理后的水体总氮、总磷含量达到地表IV类水标准。项目年处理水量约30万t,每年以较低的成本(平均水处理费用约为0.03元/t),削减总氮、总磷和氨氮量分别为1496.6 kg、176.0 kg和1408.6 kg。通过引植多种浮叶植物、挺水植物、沉水植物,该湿地修复工程为当地营造了优美的湿地景观。多水塘活水链人工湿地是集经济效益、生态效益、环境效益于一体的新型水体生态治理技术,为我国城镇黑臭河道治理提供了一条新的途径。  相似文献   
1000.
The present paper reports, for the first time, the occurrence of an omphacite‐bearing mafic schist from the Asemi‐gawa region of the Sanbagawa belt (southwest Japan). The mafic schist occurs as thin layers within pelitic schist of the albite–biotite zone. Omphacite in the mafic schist only occurs as inclusions in garnet, and albite is the major Na phase in the matrix, suggesting that the mafic schist represents highly retrogressed eclogite. Garnet grains in the sample show prograde‐type compositional zoning with no textural or compositional break, and contain mineral inclusions of omphacite, quartz, glaucophane, barroisite/hornblende, epidote and titanite. In addition to the petrographic observations, Raman spectroscopy and focused ion beam system–transmission electron microscope analyses were used for identification of omphacite in the sample. The omphacite in the sample shows a strong Raman peak at 678 cm?1, and concomitant Raman peaks are all consistent with those of the reference omphacite Raman spectrum. The selected area electron diffraction pattern of the omphacite is compatible with the common P2/n omphacite structure. Quartz inclusions in the mafic schist preserve high residual pressure values of Δω1 > 8.5 cm?1, corresponding to the eclogite facies conditions. The combination of Raman geothermobarometries and garnet–clinopyroxene geothermometry gives peak pressure–temperature (PT) conditions of 1.7–2.0 GPa and 440–540 °C for the mafic schist. The peak P–T values are comparable to those of the schistose eclogitic rocks in other Sanbagawa eclogite units of Shikoku. These findings along with previous age constraints suggest that most of the Sanbagawa schistose eclogites and associated metasedimentary rocks share similar simple P–T histories along the Late Cretaceous subduction zone.  相似文献   
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