贵州织金磷矿岩元素地球化学特征

采用电感耦合等离子体-质谱仪(ICP-MS)对贵州织金戈仲伍剖面戈仲伍组磷矿岩样品的微量、稀土元素含量进行了测定。戈仲伍组磷矿岩主要为生物碎屑白云岩、硅质磷块岩,普遍形成生物碎屑结构,以小壳类动物化石及藻类化石为主。分析结果表明,磷矿岩中As、Sb等微量元素富集,Co/Ni的比值为0.14,明显小于1;U/Th比值介于1.27~7.39之间,平均值为3.40;在lgw(U)-lgw(Th)关系图、Cr-Zr的关系图中样品点几乎都落在热水沉积区,表现出热水沉积成因的地球化学特征。磷矿岩中普遍富集稀土元素,含稀土总量∑REE较高,尤其富集Y重稀土元素;磷矿岩具Ce负异常,指示环境处于氧化程度相对较高状态;稀土元素北美页岩标准化模式曲线为帽状形态,指示在磷矿岩形成过程中有生物或有机质参与作用;磷矿岩普遍具Eu正异常、稀土总量较高、∑LREE/∑HREE比值较高的特征,暗示戈仲伍组磷矿岩具有正常海相沉积伴有海相热水沉积混合成因的特征。     

贵州织金新华含稀土磷矿床稀土元素地球化学及生物成矿基本特征

对贵州织金新华含稀土磷矿床进行的稀土元素及微量元素分析结果表明，磷块岩中普遍富集稀土元素，稀土总量∑REE较高，并富集Y元素及La，Nd等轻稀土元素。LREE／HREE比值较高。含稀土磷块岩普遍具Ce负异常，显示其对源区的继承性。指示成磷环境处于氧化程度相对较高状态。稀土元素球粒陨石标准化模式曲线、北美页岩标准化模式曲线、Ce元素异常、LREE／HREE比值、微量元素特征及岩石矿物特征表明，织金新华含稀土磷矿床具以正常海相生物-化学沉积等为主伴有海相热水沉积混合成因的特征。在磷矿成矿过程中沉积物沉积时，活体生物及死亡残骸不同程度地摄取和富集了La，Nd，Ce等稀土元素、Y元素及其他微量元素，沉积在含磷层位，构成大量的含稀土、含生物碎屑白云质磷块岩。     

贵州织金新华含稀土磷矿床稀土元素地球化学研究

对贵州织金新华含稀土磷矿床进行的稀土元素及微量元素分析结果表明,磷块岩中普遍富集稀土元素,含稀土总量∑REE较高,并富集Y、La、Nd等重稀土及轻稀土元素.LREE/HREE比值较高,但低于上部围岩之值.含稀土磷块岩普遍具Ce的负异常,显示其对源区的继承性,也指示成磷环境处于氧化程度相对较高状态.稀土元素球粒陨石标准化模式曲线、北美页岩标准化模式曲线、Ce元素异常、LREE/HREE比值、微量元素特征及岩石矿物特征表明,织金新华含稀土磷矿床具以正常海相生物-化学沉积等为主伴有海相热水沉积混合成因的特征.文中讨论了含稀土磷块岩氧化矿石中稀土元素的迁移富集规律及特征.     

贵州织金磷矿岩稀土元素地球化学特征研究

贵州织金戈仲伍剖面戈仲伍组磷质岩主要为生物碎屑白云质、硅质磷块岩，普遍形成生物碎屑结构，以小壳类动物化石及藻类化石为主。采用电感耦合等离子体-质谱仪(ICP-MS)对戈仲伍组磷质岩样品的稀土元素含量进行测定分析，结果表明：磷质岩中普遍富集稀土元素，含稀土总量EREE较高，尤其富集Y重稀土元素；磷质岩具Ce负异常，指示环境处于氧化程度相对较高状态；稀土元素北美页岩标准化模式曲线为帽状形态，指示在磷质岩形成过程中有生物或有机质参与作用；磷质岩普遍具Eu正异常、稀土总量较高、∑LREE／∑HREE比值较高的特征，暗示戈仲伍组磷矿具有正常海相沉积伴有海相热水沉积混合成因的特征。     

贵州织金新华含稀土磷矿床矿区土壤稀土元素分布特征

稀土元素分析结果表明,贵州织金新华含稀土磷矿床矿区上层土壤中普遍富集稀土元素．其∑REE较高,但比含稀土磷块岩低．表明磷块岩在风化过程中已有部分稀土元素流失。轻稀土元素La、Ce及Y大量集中,LREE／HREE比值较高,说明岩石在风化过程中形成的粘土矿物对稀土元素有一定的吸附作用。但是粘土矿物对稀土元素的吸附量小于REE易溶配合物的流失量。稀土元素球粒陨石标准化模式曲线及Ce异常等特征表明,织金新华含稀土磷矿床矿区土壤中稀土元素分配模式继承了原岩特征。     

贵州织金磷块岩型稀土矿含矿岩系REE地球化学特征与稀土富集

贵州织金下寒武统戈仲武组(?1gz)磷矿富集大量稀土,但是磷块岩中REE富集机制问题尚不清楚。本文对贵州织金不同稀土含量区间(262×10~(-6)、262×10~(-6)～527×10~(-6)、527×10~(-6)～761×10~(-6)、761×10~(-6))的磷块岩的研究表明,磷块岩的稀土配分均显示出Ce负异常、Eu无明显异常、MREE富集以及富集重稀土元素Y的特征。(La/Sm)N-δCe及δPr-δCe图解显示织金磷块岩Ce异常为真实的Ce异常,代表磷块岩形成在氧化环境。但当时海水的氧化环境并不是控制MREE富集的决定因素。(La/Sm)N-SmN、(Gd/Yb)N-YbN散点图显示MREE富集是稀土在富集过程中稀土发生分异的结果。(Dy/Sm)N-δEu散点图以及Eu无明显异常说明织金磷块岩形成过程中可能无热水作用的参与。地史时期"老磷块岩"普遍存在重稀土亏损的特征。     

黔北桑木场背斜灯影组热液白云岩稀土元素地球化学特征

本文利用电感耦合等离子体质谱仪,分析了习水桑木场背斜核部铅锌矿赋矿热液蚀变白云岩的稀土元素组成,并初步探讨了白云岩化与铅锌矿化间的关系。铅锌矿体旁侧工程中白云岩样品的测试显示:有部分样品Zn含量超过200×10-6,具有矿化显示;全部样品∑REE很低(∑REE=0.82～5.96×10-6),具有明显的Ce负异常(δCe=0.37～0.68),除个别有矿化显示的白云岩样品具有正Eu异常(δEu=1.15～2.40)外,其余样品均具有负Eu异常(δEu=0.56～0.80)。在稀土元素球粒陨石标准化配分模式图上,全部样品均呈现轻稀土富集特征。综合研究,认为白云岩化热液流体具有轻稀土富集及Eu和Ce负异常特征,而氧化还原环境的变化可能是导致本区铅锌矿化的重要因素。     

贵州道坨锰矿菱锰矿的稀土元素特征

贵州道坨锰矿是2010年发现的一个大型碳酸锰矿床,含矿层位为南华系大塘坡组底部的含锰黑色页岩,主要含锰矿物为菱锰矿。通过对锰矿石全岩与提取出的菱锰矿进行稀土元素对比分析发现:(1)不同Mn含量的锰矿石的∑REE在(171.84~243.08)×10-6之间,提取的菱锰矿的∑REE在(32.52~135.69)×10-6之间,菱锰矿的∑REE占全岩∑REE的比例从15%到80%不等。菱锰矿的∑REE随着锰含量的升高而升高,且稀土元素配分模式都呈轻稀土含量少,中稀土富集,重稀土相对中稀土减少的"帽"式配分模式,而全岩的配分模式基本是平坦的直线型。随着全岩中Mn含量的升高,全岩和菱锰矿的配分模式越来越相似;(2)菱锰矿的δCe值在1左右,且随着Mn含量的升高。δCe值变大,这可能是因为Ce在锰氧化物或氢氧化物逐渐沉积富集的过程中,逐渐地被吸附,而造成了异常值的逐渐增大,说明菱锰矿的形成经过了锰氧化物或氢氧化物的阶段;(3)分别比较菱锰矿中Mn和P与轻、中、重稀土的相关性,Mn与中稀土的相关性最差,而P与中稀土的相关性最好。因此菱锰矿所表现出的中稀土富集的现象可能是其中的磷酸盐引起的,而磷酸盐与菱锰矿的共存可能是因为当时环境中磷与锰的分离不彻底造成的。     

黔北铝土矿稀土元素富集机制——以新民铝土矿为例

通过对黔北新民铝土矿岩矿石稀土元素的系统分析,探讨了黔北铝土矿稀土元素特征与富集机制。研究发现:黄龙组灰岩呈"平坦型"稀土元素配分模式,韩家店群泥岩、梁山组炭质泥岩及大竹园组(含矿岩系)呈"右倾型"轻稀土富集特征,而大竹园组随着风化作用的增强从陡"右倾型"的铝质泥岩→缓"右倾型"的豆状、致密块状、碎屑状铝土矿→缓"左倾型"土状铝土矿的特征。且含矿岩系由底到顶,∑REE具减少趋势,顺着其倾向∑REE有下降趋势,沿着走向其有升高趋势;这受到不同底板岩性及厚度大小的影响,底板泥岩比灰岩更易使含矿岩系富集稀土,同为灰岩,其厚度越大其稀土总量有富集趋势。而∑REE受到矿物组合(岩性)控制,其有"含独高稀,鲕粒富稀,豆状少稀,高铝贫稀"特征。对实验数据进行分析和做相关性图解(Sr/Ba—∑REE、Sr/Cu—∑REE、δCe—∑REE、δEu—∑REE)可知,在干热气候的海相咸水环境更易使稀土富集,虽含矿岩系主要是在氧化环境中形成,但高∑REE样品易在还原环境中富集。     

贵州织金磷块岩型稀土矿地球化学特征

贵州织金磷块岩型稀土矿产于梅树村期戈仲伍组含磷地层,现探明资源量350万吨,其中Y元素占30%以上,为超大型稀土矿床。本文选取4个典型钻孔、一处露头和一采矿坑进行采样,并利用扫描电镜、电子探针、X荧光光谱、和电感耦合等离子体质谱仪对样品的矿石特征和地球化学特征进行了分析。结果表明,稀土元素主要富集于戈仲武组下部的砂屑磷块岩和具层纹构造磷块岩的深色部分,不以独立矿物形式存在,而与磷灰石关系密切。从Fe/Ti、(Fe+Mn)/Ti、Al/(Al+Fe+Mn)比值,As和Sb富集情况,U-Th关系,稀土元素配分模式,δEu异常情况,均反映含矿岩系具有热水沉积成因特征,综合分析认为,戈仲伍组富稀土样品具有热水和风化特征,稀土富集可能与热水沉积或风化改造有关。     

Global repeating events in the history of the Earth and the motion of the Sun in the Galaxy

Chronological analyses of correlations between certain global repeating events (mass extinctions of marine organisms, meteorite impacts, and flashes in the frequency of geomagnetic reversals) during the Phanerozoic Eon and the motion of the solar system in the Galaxy are presented for five rotationally symmetrical models for the regular Galactic gravitational field. Thirteen of sixteen mass-extinction events can be described by a repetition interval of 183±3 million years. This is in agreement with the anomalistic period (interval between two subsequent passages of the Sun through the apocenter of its Galactic orbit) in the model of Allen and Martos. The positions of the minima and maxima in Gaussian functions approximating the frequency distribution for geomagnetic reversals also agree with the times of passage of the Sun through the apocenter and pericenter, respectively, of its Galactic orbit in this model. The maximum in the distribution of the deviations of the dates of mass extinctions from the nearest dates of impacts of large, crater-forming bodies is close to zero, providing evidence that many such events are correlated. As a rule, extinctions follow impact events. The impacts of large bodies have occurred most often when the solar system passes through the Galactic plane, while mass extinctions occur more often at some distance from the Galactic plane (about 40 pc). As a rule, intervals of increases in the frequency of geomagnetic reversals coincide with dates of impacts of large bodies. At the same time, these intervals do not show a clear correlation with the dates of mass extinctions. The intensity of mass extinctions, like the energy released by impacts, is consistently higher in periods when the Sun is moving from the apocenter toward the pericenter of its orbit, than when it is moving from the pericenter toward the apocenter. Thus, there is evidence for a variety of relationships between repeating global events in the Phanerozoic and the motion of the Sun in the Galaxy. Long-period variations in the frequency of geomagnetic reversals are correlated with the orbital motion of the Sun, and increases in the frequency of geomagnetic reversals are correlated with impacts. Mass extinctions are correlated with the impacts of large bodies, whose motions may have been perturbed by clouds of interstellar material concentrated toward the Galactic plane and by the shock front associated with the Perseus spiral arm, through which the solar system passes. The velocity of the Sun relative to the spiral pattern is estimated.     

截潜工程在计算山前侧向补给量中的应用

在计算山前侧向补给量的方法中,最常用的就是达西断面法,但达西断面法需要获取较多的参数,对于山前无钻孔或只有少量钻孔且水文地质研究程度较低的区域,很难采用达西断面法来计算得到山前侧向补给量。对于无法运用达西断面法但存在完整式截潜工程的山丘区,可以结合完整式截潜工程的截潜量利用水量均衡法计算山前侧向补给量。     

"青藏高原南部空白区基础地质调查与研究"计划项目新成果、新进展

通过2004年度各相关图幅的大力工作，在基础地质、矿产和资源等方面取得了大量实际材料，综合研究区域构造．地层格架、青藏高原地质图和青藏高原南部火山岩及其地球动力学意义等，取得重要进展和新认识，在矿产资源、旅游和人文景观等方面也取得重要阶段性成果。     

“青藏高原南部空白区基础地质调查与研究”计划项目新成果、新进展

通过2 0 0 4年度各相关图幅的大力工作,在基础地质、矿产和资源等方面取得了大量实际材料,综合研究区域构造地层格架、青藏高原地质图和青藏高原南部火山岩及其地球动力学意义等,取得重要进展和新认识,在矿产资源、旅游和人文景观等方面也取得重要阶段性成果。     

关中盆地大荔地区地下水氟水文地球化学规律

为了研究关中盆地大荔地区氟的水文地球化学规律,采集239个地下水样品及35个土壤样品,分析了水化学类型和水化学组分对氟的影响,结果表明在弱碱性环境下,重碳酸钠型是促进氟富集并增强围岩向地下水中转化的主要因素;硫酸钙镁型的地下水抑制氟富集。水化学组分中Na+、Cl-、HCO3-、pH与氟呈正相关,而Ca2+则抑制水溶液中氟含量增加;迁移系数与HCO3-、pH呈正相关关系,与其他主要离子呈负相关关系。利用Preeqic软件分析了饱和指数和Ca2+、F-的离子活度,得出萤石的平衡控制着氟和钙的水文地球化学行为,F-可能来源于萤石和方解石的分解。     

Determination of Emissions in the City by the Rate of Change in the Integral Content of Impurities in the Atmospheric Boundary Layer

Doklady Earth Sciences - A new approach to the problem of determining the density of emission fluxes of anthropogenic impurities from distributed urban sources by the rate of growth of the integral...     

Terrane tectonics in the formation of the groundwater runoff in the active water-exchange zone of mountainous river valleys in the cryolithozone

The significant role of the drainage area’s geological background in the formation of the groundwater runoff in the active water-exchange zone was revealed for the first time on the basis of long-term observations of streams of the Upper Kolyma River region during the autumn-winter low-water period, when the rivers are fed only by the groundwater recharge. The analysis of all the available data made it possible to define the characteristic periods in the autumn-winter low-water season. The waters of the seasonally thawed layer play the dominant role in the river’s recharge in September; the suprapermafrost water, in January; and the subgelisol water (nonfreezing water streams) during the 30-day-long period of the minimal flow. The quantitative parameters of the groundwater runoff corresponding to its module during this period reflect the water influx to the active water-exchange zone. It is established that the latter is minimal in the In’yali-Debin synclinorium, which consists of sedimentary rocks formed in deepwater trough environments. Their subsequent transformation proceeded under the action of subduction-accretionary and shear strains. The water availability in the active water-exchange in the Ayan-Yuryakh anticlinorium zone is substantially higher, although the Late Paleozoic and Early Mesozoic sedimentary formations of this area were also deposited in deepwater trough settings, but their subsequent evolution was related to the uplift of the anticlinorium. The maximal watering is observed in the active water-exchange zone of the Omulevka terrane, which is composed of Paleozoic terrigenous-carbonate and carbonate formations. The differences in the hydrogeological regimes of the terranes may be significant with respect to their geoecology.