庐枞盆地泥河铁矿床成矿岩体三维形态学分析及找矿指标研究

泥河铁矿床位于长江中下游成矿带内庐枞盆地的西北部,属玢岩型铁矿床,前人对该矿床的基础地质研究已有一定成果,积累了大量的数据资料,表明泥河铁矿床的形成与辉石闪长玢岩顶面形态关系密切。本文选择泥河铁矿床闪长玢岩为研究对象,以钻孔资料为依据,采用离散光滑插值法建立成矿岩体的精细三维模型,重现了闪长玢岩体的形态特征,将三维模型离散化后提取岩体顶面并通过三维形态分析方法进行数值分析,提取了岩体表面的隆起、凹陷形态,并与已知矿体进行对比,验证了该矿床成矿岩体隆起形态与矿体位置的对应关系。本文通过多次实验确定最佳表达的滑动窗口尺寸和与成矿岩体形态有关的找矿指标,结果证明利用10×10个单元的滑动窗口可以识别80%以上矿体。本文对三维成矿预测中三维空间分析方法进行探索,证明成矿岩体三维形态分析方法的有效性,这一方法可直接应用于与泥河铁矿床类似的玢岩型铁矿床三维成矿预测中。     

胶北地块与金成矿有关的郭家岭岩体和上庄岩体年代学及地球化学研究

胶东半岛是我国最主要的原生金矿矿集区,金矿的主要控矿围岩是郭家岭花岗岩,通过研究郭家岭花岗岩的地球化学特征对研究金矿的成因和物质来源具有指示性意义。本文研究的两个花岗岩岩体为上庄岩体和郭家岭岩体,两岩体同属郭家岭型花岗岩。通过对两岩体的花岗岩样进行岩相学矿相学观察、全岩主、微量元素和U-Pb同位素分析,获得胶东半岛中生代岩浆岩的成因机制与源区性质及自然金的产出形式等科学信息。LAICP MS锆石U-Pb年龄得出郭家岭岩体年龄125.4±2.2 Ma,上庄岩体U-Pb年龄128.8±2.0 Ma,都为中生代早白垩世,两岩体年龄相差3Ma,在年龄误差范围来看可以把两岩体作为同一期岩体,也在年龄角度证实两岩体都同属郭家岭花岗岩。两岩体的锆石组成都含有太古宙和晚侏罗纪的继承锆石,指示两岩体的成岩物质来源具相似性,都包含太古宙岩石成分和晚侏罗世花岗岩成分。两岩体具有相似的稀土元素和微量元素分配模式,表现出明显的LREE富集和HREE极度亏损,没有明显的铕负异常。郭家岭岩体和上庄岩体花岗岩都具有类似埃达克岩的特征,都具有高的Sr含量(913×10-6~1325×10-6),低的Y含量(2.2×10-6~8.4×10-6)和Yb含量(0.21×10-6~0.68×10-6),较高的(Dy/Yb)N比值1.62~2.28,暗示花岗岩岩浆形成时石榴石是一个重要的残留相,而没有斜长石作为残留相。两岩体具有较低的MgO、Cr、Ni含量和Mg#,反映郭家岭型花岗岩岩浆的形成可能是岛弧环境榴辉岩相压力条件下洋壳玄武质岩石的部分熔融。     

面向道路网络地图示意化的线形简化方法

针对当前示意网络地图线形状简化方法中存在需要人工干预或地图认知度低的问题,本文提出自动化程度高并能保证良好地图认知的线形状简化方法.该方法通过合理设定线形状简化中所需的阈值以避免人工干预,提高了线形状简化过程的自动化程度,并通过在简化过程中应用平滑算法,以减少示意结果中线对象在方向上的转折数,从而提高了简化度和清晰度.试验表明该方法不仅可以生成清晰的示意结果,并且能够保证良好的地图认知度.     

星康吉鳗精子的超微结构研究

为探讨星康吉鳗(Conger myriaster)精子的超微结构和形态,应用扫描电镜和透射电镜对星康吉鳗精子结构进行观察。结果表明,精子由头部、中段和鞭毛3部分组成,有其独特的结构,总长度为35.75± 1.15µm。精子头部为新月形,主要由细胞核构成,细胞核内有核泡,无顶体结构。精子头部的质膜内包含单一的线粒体。精子头部长为3.33±0.16 um,头宽为1.12±0.13 um。在精子头部的凸面上,有4条从中段到头端的条纹。精子中段伸出一支根,支根位于精子的中段末端。精子中段长度为0.55±0.05 um,支根长度为1.38±0.08 um、直径为90.48±6.06 nm。精子尾部鞭毛细长,鞭毛横切面呈圆形,无侧鳍,鞭毛的轴丝结构为“9+0”型;一些鞭毛的末端呈现卷曲状,发育机制尚不明确。精子鞭毛长为31.16±1.51µm,鞭毛直径为0.17±0.01µm。通过比较分析发现精子的这些形态学特征不仅表现在星康吉鳗精子,还表现在鳗鲡目其他属的精子;表明是鳗鲡目精子的共同特征。本研究揭示了星康吉鳗精子的形态结构,为突破星康吉鳗人工繁殖技术提供了理论参考。     

On the hydraulic intake shape factor for a circular opening located at an impervious boundary: Influence of inclined stratification

In this paper, we develop an exact closed form solution for a circular entry point located at the interface between an impermeable material and a stratified porous medium, where the principal plane of hydraulic isotropy is inclined to the interface. Copyright © 2010 John Wiley & Sons, Ltd.     

Developing the tools for geological shape analysis,with regional‐ to local‐scale examples from the Kalgoorlie Terrane of Western Australia

Geological map data are often underused in mineral‐exploration programs, which rely increasingly on regolith geochemistry and geophysical and other remotely sensed data to generate exploration targets. However, solid geology maps, which are progressively being upgraded due to improved interpretations of superior, remotely sensed images and airborne geophysical data, can be useful in targeting specific types of mineral deposits, which formed late in the evolutionary history of the host terrane. In such terranes, the present map geometry is essentially the same as that at the time of deposit formation. This is the case for orogenic lode‐gold deposits, which commonly show predictable structural controls and/or structural geometry. Thus, the shape of a rock body, or combinations of structures and rock bodies, may provide an important guide to the exploration potential for orogenic lode‐gold deposits. However, until recently, there has been a dearth of techniques to quantify the various properties of shape, and hence test the potential of the two‐dimensional shape of geological bodies in map view as an exploration tool. Integrating techniques from the field of pattern recognition with a modern Geographical Information System (GIS) can provide the shape‐analysis tools required to investigate the geometries of geological shapes. Two‐dimensional shape analysis is now possible through the calculation of several shape metrics including, but not restricted to, aspect ratio, blockiness, elongation, compactness, complexity, roundness, spreadness and squareness. Methods are developed for describing the geometries of rock units about mineral deposits, or any geological features, at any scale, which for the first time makes it possible to compare shapes. These shape‐analysis techniques are tested using orogenic lode‐gold deposits, particularly those in the Kalgoorlie Terrane of the highly auriferous Late Archaean Norseman‐Wiluna Belt of Western Australia. On a global scale, shape analysis indicates that those greenstone belts whose volcanic rock sequences have high elongation and relative low roundness, complexity and aspect ratio (e.g. Kalgoorlie Terrane) are likely to be the most richly endowed in gold. On a more local scale, characteristics of the shape of geological features around the Golden Mile deposit are calculated and used to test the likelihood of occurrence of gold deposits with similar geometry elsewhere in the Kalgoorlie Terrane. The area with the most closely matching shape, on the basis of a 2 km clipping‐circle radius, chosen on the basis of available proximity‐analysis data, corresponds to the recently discovered Ghost Crab deposit, illustrating the potential of the shape analysis methodology in mineral exploration. Shape analysis is, at least in part, scale dependent, due to the inherent problem of being able to define rock boundaries more precisely in units that have strong geophysical signatures than those with weak signatures in poorly exposed terranes. Overcoming this problem is a challenge to the application of this methodology.     

Geopotential from space techniques

The monitoring of the perturbed motion of artificial satellites since the 1960's has provided a valuable resource for improved activities in geodesy. These observations and the improved geodetic techniques they fostered have provided an unparalleled means for studying both the gravity field and the Earth's shape. In this paper, we will review the various determinations of the Earth's gravity field produced at many research centers over the years from space techniques. The specific methods which have been used to measure our planet, such as satellite altimetry and satellite orbital perturbation analyses (over short and long periods of time), will be compared.     

扬子陆块西缘中元古代晚期元谋花岗岩的时代、成因及构造意义

扬子陆块西缘晚中元古代地质演化史一直存在较大争议,本文选择以扬子西缘元谋杂岩中一套二长花岗岩为研究对象,开展岩相学、锆石U-Pb年代学、全岩地球化学等综合研究,为认识和理解扬子西缘晚中元古代地质演化提供支撑。两件元谋二长花岗岩样品的LA-ICP-MS锆石U-Pb年龄分别为1086±10 Ma（MSWD=1.4,n=50）和1099±10 Ma（MSWD=1.8,n=58）。所有样品具有高硅（SiO₂为69.44%~73.98%）、富碱（Na₂O+K₂O为6.11%~7.72%）、贫钙（CaO为0.39%~1.46%）、贫镁（MgO为0.52%~0.76%）、低钛（TiO₂为0.30%~0.59%）的特点,同时表现出强过铝质（A/CNK=1.19~1.35）及中钾钙碱性–钾玄岩系列特征。它们具有高的稀土元素总量（∑REE=211.60×10^-6~349.01×10^-6）,呈现轻稀土元素富集和重稀土元素亏损（（La/Yb）_N=4.32~7.36）;富集Rb、U、Th等大离子亲石元素和Zr、Th、Hf等,亏损Nb、Ta、Ba等元素,并具有明显的负Eu异常（δEu=0.46~0.59）,锆石饱和温度介于827~912℃之间,展示了A型花岗岩的属性。这些二长花岗岩可能是通过中上地壳的中酸性火成岩的部分熔融形成,结合前人的研究成果,它们最可能形成于弧后的伸展环境,综合扬子陆块周缘晚中元古代的岩浆记录,元谋杂岩中1.09 Ga二长花岗岩的形成应与扬子陆块开始参与Rodinia超大陆聚合有关。     

扬子陆块北缘构造演化新认识：来自原花山群年代学和地球化学的制约

原花山群分布于紧邻南秦岭的扬子陆块北缘大洪山地区,出露于重要的构造部位,是研究其形成时期扬子陆块构造演化及其与南秦岭关系的重要载体,其物质组成、形成时代和构造属性长期存在争论。本文将原花山群解体为花山构造混杂岩和正常的火山—沉积地层（本文所指花山群）两部分来讨论。笔者重新厘定了花山群的沉积时限,有针对性地对有构造背景争议的花山群进行玄武岩地球化学研究,对有时代争议的混杂岩进行锆石U-Pb年代学研究。年代学、地球化学和沉积学综合研究表明,花山群的沉积时限为ca. 830 Ma至ca. 800 Ma,形成于与Rodinia超大陆裂解有关的陆内裂谷盆地。花山构造混杂岩带可能不只是晋宁期的缝合带,而是具有多期物质组成、经历了多期构造叠加的复合型缝合带。结合他人成果,我们提出了扬子陆块与南秦岭从新元古代到早古生代的构造演化新模式。     

中祁连地块西段青白口系其它大坂组英安质凝灰岩LA- ICP- MS锆石U- Pb年龄及其地质意义

新元古界青白口系其它大坂组是中祁连地块西段基底岩系之一,对研究中祁连地块元古宙地质构造演化具有重要意义。笔者等通过1∶5万区调工作在其它大坂组中发现了英安质晶屑岩屑凝灰岩夹层,并对凝灰岩进行了锆石U-Pb年代学、岩石地球化学研究。测年结果表明样品中锆石年龄主要分3组。结合区域地质资料,笔者等认为第一组锆石(1456～1524 Ma)和第二组锆石(1018～1021 M)为外来锆石或/碎屑锆石,分别为物源区中元古代早期Columbia超大陆裂解事件和Rodinia大陆聚合事件(格林威尔造山作用)在中祁连地块中的响应;第三组锆石(946～964 Ma)的n(²⁰⁶Pb)/n(²³⁸U)加权年龄为958±3 Ma(MSWD=1.4),代表英安质凝灰岩的形成时代。岩石地球化学分析表明,其它大坂组英安质晶屑岩屑凝灰岩样品属于过铝质(A/CNK=1.37～1.75)、高钾(K₂O>Na₂O,K₂O=4.48%～4.86%)、钙碱性(σ=0.89～1.26)火山岩,稀土总量为(149....