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91.
J.N. Hutchinson 《Proceedings of the Geologists' Association. Geologists' Association》2010,121(4):444-454
Exposures on Wimbledon Hill, SW London, in the Palaeogene London Clay Formation, are described. The 3° slopes are mantled by clayey solifluction (head) deposits, comprising two superimposed sheets, each around 1.2 m thick. The lower sheet exhibits relict sand wedges forming polygons 1.0-1.5 m across, up to 50 mm wide and 1.25 m deep. These have no surface expression. The wedges are sand-filled and modify significantly the hydrogeology and properties of the solifluction mantle. There are no sand wedges in the upper solifluction sheet.The mechanics of emplacement of the lower solifluction sheet are explored and the high initial water content estimated. Subsequent desiccation and consolidation have reduced the thickness of this sheet by at least 35%, thus distorting contained features such as the wedges. An active layer about 0.4 m thick is inferred to have formed in the top of the lower solifluction sheet. No direct dating was undertaken but, by analogy with relevant dated sites in southern Britain and the Netherlands it is inferred that the lower solifluction sheet was emplaced during the first part of the Loch Lomond Stadial and frost-cracked during a subsequent, colder and more arid part. On this basis, following filling of the cracks by sand, emplacement of the upper solifluction sheet would have occurred in the later part of the Loch Lomond Stadial. 相似文献
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93.
This work benefited from a comprehensive set of logging and mineralogical data that was acquired from the 2-km-deep EST433 borehole of Montiers-sur-Saulx (Meuse, France). A multiple linear regression analysis was performed on three sets of data: (a) sonic data (P- and S-wave velocities), (b) total combinable magnetic resonance (TCMR) porosity data, and (c) X-ray diffraction (XRD) data. The analysis was performed to estimate the clay content in the Callovo-Oxfordian (COx) claystone and other clay-rocks of the stratigraphic column. The inferred statistical relationships were compared to results obtained from a conventional spectral gamma ray (GR) approach.The results indicate that simple linear regressions using only elastic wave velocities (a) accounted for more than 81% of the vertical variability of the clay content in the COx formation (i.e., coefficient regression R2 values greater than 81%) and (b) enable the estimation of clay content with the same accuracy as the spectral GR approach. Both approaches, our acoustic regressions and spectral GR methodology, provide estimate errors that are within the range of uncertainties associated with the XRD analysis applied. Moreover, using the whole set of XRD data showed that the elastic wave velocities and the TCMR porosity as explanatory variables are better predictors of total clay content than swelling clay mineral content.Blind estimations of clay content were performed using data acquired in clay-rocks from the same stratigraphic column and in the COx formation located a few kilometers distant in the EST423 borehole. The results demonstrated that the established regressions must be used with caution when vertically and horizontally extrapolating the estimated clay content. This difficulty is partly explained by the influence of the microstructure of the studied clay-rocks, which was insufficiently taken into account via the petrophysical variables considered in this work. 相似文献
94.
An account is given of a Geologists’ Association meeting in the Isle of Purbeck held on 28th–30th September 2012 and the stratigraphy and structures of the rocks examined during the weekend are described. Uppermost Jurassic Stage nomenclature and recent changes to stratigraphical nomenclature in the uppermost part of the Kimmeridge Clay Formation are discussed and the conclusion reached that the long-established divisions (Members) of this Formation are both readily recognisable and have nomenclatorial priority. The recent change to the position of Pallasioides-Rotunda zonal boundary ignores the ammonite fauna and is inappropriate. For the Lulworth district the stratigraphy of the uppermost Jurassic (Portlandian) through Lower and Upper Cretaceous formations are described and their associated structures discussed. The coastal evolution of the Lulworth coast is briefly discussed. 相似文献
95.
本文以智博铁矿区内的安山岩为研究对象,通过详细的野外地质调查,并利用电子显微镜和电子探针,对安山岩中的主要矿物进行了系统的岩相学观察和矿物学研究。研究表明,智博安山岩中斜长石主要为Na-高钠长石,具低TiO2,高Na2O和Al2O3的特点;辉石主要为普通辉石,具高TiO2,高Al2O3的特点;角闪石主要为镁角闪石和阳起石,具低TiO2和Al2O3,高MgO的特点;副矿物磁铁矿具高TiO2,低MgO和Al2O3的特点。辉石、角闪石矿物化学特征表明,智博铁矿安山岩的母岩浆属于壳幔混源的玄武质岩浆,构造环境为火山岛弧环境。智博安山岩中单斜辉石结晶温度为1225℃左右,结晶压力约0.795GPa,结晶深度约26km。智博铁矿后期的热液作用也参与了磁铁矿成矿,对智博铁矿的成矿有一定的贡献。 相似文献
96.
铁木里克铁矿是西天山阿吾拉勒成矿带上一个高品位的磁铁矿矿床,赋存于石炭纪大哈拉军山组火山岩中。矿区围岩蚀变较弱,主要以低温热液阶段的绿泥石化和绿帘石化为主。根据野外矿石组构以及镜下观察,该矿床可以划分为四个成矿阶段。目前该矿床的研究程度较低,矿床成因存在较大争议。磁铁矿和赤铁矿的电子探针结果显示,该矿床的形成与岩浆-热液系统密切相关;辉石和角闪石的电子探针结果显示,辉石未发生蚀变,只有角闪石轻微地发生了阳起石化。矿石中的黄铁矿硫同位素(0.1‰~2.9‰)显示具有深源地幔特征,磁铁矿的氧同位素(-2.7‰~0.5‰)暗示岩浆热液对成矿具有重要作用,以及成矿晚期低温热液过程对早先形成的磁铁矿起到了改造作用。结合区域铁矿带的成矿地质特征,本文认为铁木里克铁矿的形成主要与岩浆-热液系统密切相关,在大量磁铁矿形成之后,有少量成矿流体与海水混合,对矿床和围岩进行了低温热液蚀变,形成了充填在磁铁矿矿石气孔中的赤铁矿和黄铁矿。 相似文献
97.
张家洼矽卡岩型铁矿位于华北克拉通东南部,赋存在石炭系本溪组与奥陶系马家沟组之间的假整合面处及闪长岩体与奥陶系马家沟组大理岩的接触带附近,富铁矿石资源量已达大型规模。研究发现矽卡岩矿物种类在内外接触带分布有一定区别,内带为石榴石等钙质矽卡岩矿物,而外带为阳起石、金云母等镁质矽卡岩矿物,整体构成钙镁质矽卡岩。对矽卡岩矿物系统的研究表明,透辉石及石榴石发育有环带,其氧化物含量随矿物环带的形成比例不断变化,暗示酸碱度及氧逸度随着成矿流体的演化而发生相应的变化,即由早期矽卡岩阶段的相对还原的酸性环境演化为退化蚀变阶段相对氧化的碱性环境从而导致铁质逐渐萃取多次富集、沉淀,后期随着磁铁矿的沉淀又逐渐在硫化物阶段转化为还原环境生成金属硫化物。 相似文献
98.
鸡笼山金矿是长江中下游鄂东南地区典型的矽卡岩金矿床,其矽卡岩矿物学特征研究较少。围岩为三叠纪大冶组灰岩和白云质灰岩,决定了该矿床发育丰富的矽卡岩矿物组合,主要包括石榴石、透辉石、硅灰石、绿帘石、金云母等。本文详细研究了不同阶段矽卡岩的矿物学特征,并对其进行了电子探针分析(EMPA)。结果表明石榴石属于钙铝-钙铁系列,辉石为透辉石,以钙铁榴石-透辉石共生的富金矽卡岩组合是在较高氧逸度和较低酸度条件下形成的,具有铜金矿的成矿专属性。伴随着流体的演化,矽卡岩与矿体在时空和成因上都具有密切的联系。结合矿区内发育有斑岩型矿体,暗示鸡笼山金矿床可能具有统一的斑岩-矽卡岩型成矿系统,深部具有很大的找矿潜力。 相似文献
99.
100.
The mobility, bioaccessibility and transfer pathways of metals and metalloids in estuarine sediments have been the focus of much detailed research. However, to date, few studies have examined the mineralogical siting of metals and metalloids in such sediments. This is despite the fact the mineralogy of sediments is an important factor that controls which and how much of a particular metal is released to pore waters and overlying water columns. This study reports on the mineralogical siting of metals in contaminated estuarine sediments, Hobart, Australia, and aims to evaluate the mobility of metals in the contaminated substrates. Mineralogical, mineral chemical and bulk chemical analyses demonstrate that the sediments contain very high levels of several metals and metalloids. The contaminated sediments have concentrations of zinc (Zn), lead (Pb), copper (Cu) and cadmium (Cd) ranging from 0.55 to 4.23 wt%, 0.16 to 0.70 wt%, 415 to 951 mg/kg and 23 to 300 mg/kg, respectively. Franklinite and lesser sphalerite are the main repositories of Zn, whereas much of the Pb and Cu is hosted by sulfides, organic matter and undetermined iron (Fe) oxides. While the release of contaminant loads from franklinite through dissolution is likely to be insignificant, even small releases of metals from the highly contaminated sediments can still cause the deterioration of local water quality. The contaminated sediments represent long-term sources of metal pollutants, particularly Zn, to local waters. This study demonstrates that mineralogical analyses are a vital tool to recognise the potential mobility of trace metals in estuarine environments. 相似文献