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鄂尔多斯盆地东胜区直罗组砂岩中烃类流体特征与铀成矿关系 总被引：2，自引：0，他引：2
通过对鄂尔多斯盆地东胜地区纳岭沟、大营铀矿床直罗组下段砂岩中139个样品的酸解烃分析,探讨了酸解烃中烃类气体组成特征、成因及来源,并结合该区铀矿地质特征初步分析了烃类流体与砂岩型铀成矿关系。研究结果表明,直罗组下段砂体中CH_4及C_2+含量具有从含矿砂体、灰色砂体、灰绿-绿色砂体逐渐变小的分布特征,表明该区铀成矿与烃类气体关系密切。酸解烃中气体组成特征参数C_1/ΣC、C_1/C_2~+、C_2/iC_4、C_2/C_3、iC_4/nC_4、iC_5/nC_5、ln(C_1/C_2)、ln(C_2/C_3)及δ~(13) C_(CO_2)特征表明,中侏罗统直罗组下段砂岩层中烃类气体为有机成因的油型气,烃类气主要处于成熟—高成熟阶段,是原油裂解气与原油伴生气的混合气。通过气源对比分析认为,直罗组下段砂体中的烃类气主要来源于上三叠统延长组深湖—半深湖相腐泥型烃源岩。这些原油裂解气和原油伴生气的混合气主要沿深大断裂、微裂缝等其他运移通道向上运移到直罗组砂岩中,直罗组下段砂体褪色蚀变(漂白)和绿色蚀变均是深部逸散到该层位中的烃类气体对岩石发生蚀变作用的结果,靠近断裂的直罗组下段褪色蚀变砂岩与绿色蚀变砂岩之间的氧化-还原过渡带是该区砂岩型铀矿找矿的重点方向。 相似文献
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鄂尔多斯盆地南部中侏罗统直罗组下段砂岩中已发现店头砂岩型铀矿床及多个铀矿点,但对于盆地南部直罗组沉积相研究较为薄弱,制约了砂岩型铀矿的进一步找矿工作。通过剖面实测、岩心编录,结合石油、煤炭、核工业地质钻孔资料,对鄂尔多斯盆地南部直罗—店头地区直罗组沉积特征进行精细刻画。在此基础上,探讨了沉积相与铀成矿的关系及下一步找矿方向。结果显示,直罗组下段砂体厚度30~65 m、砂地比在0.6~0.75之间,为砂质辫状河沉积。直罗组上段早期砂体厚度10~38 m、砂地比值在0.15~0.45之间,为曲流河沉积;直罗组上段沉积晚期研究区位于湖盆中心所在位置,为滨浅湖沉积。沉积环境、沉积相、辫状河河道交汇部位、砂体厚度、沉积物粒度及泥岩夹层对铀成矿具有重要控制作用。直罗组下段辫状河河道交汇或分叉部位应作为勘查重点,心滩亚相的含炭屑、黄铁矿砂质碎屑岩可作为铀矿化的找矿标志。 相似文献
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初步探讨鄂尔多斯盆地东胜铀矿田成矿作用研究若干问题 总被引：1，自引：0，他引：1
随着973项目和北方砂岩型铀矿调查工程的深入开展,笔者从中侏罗统直罗组成岩过程对铀成矿影响的角度,初步探讨了鄂尔多斯盆地东胜铀矿田成矿作用的若干问题,主要表现在以下几个方面:(1)鄂尔多斯盆地北部的古元古代孔兹岩带为东胜铀矿田中主要含铀地层-中侏罗统直罗组碎屑物、预富集铀的主要蚀源区;(2)直罗组在同生沉积过程中预富集的大量铀,为铀成矿提供了主要铀源;(3)早成岩作用下,直罗组沉积建造水将分散的、预富集的铀迁移至灰色砂岩中富集成矿,为成矿流体;(4)基于铀矿体产状及铀矿物与载铀介质的空间关系,成矿时期应为早白垩世末期,受直罗组早成岩作用制约。 相似文献
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笔者以鄂尔多斯盆地东胜铀矿田的典型矿床——纳岭沟铀矿床为主要研究对象,通过铀矿体及围岩岩石地球化学、电子探针及稳定同位素测试等方法,综合分析了东胜砂岩型铀矿田的铀源及其地质意义。结果表明:主要含矿目标层中侏罗统直罗组在同生沉积过程中,铀预富集达212.45×10~(-6),围岩达41.34×10~(-6);预富集铀主要来自于盆地北缘蚀源区;铀矿体及围岩REE配分曲线总体具一致性,右倾,个别δEu正异常,富集重稀土,两者铀源具一致性;含铀砂岩δ~(13)C_(V-PDB)=-9.7‰,δ~(18)O_(SMOW)=18.9‰,黄铁矿δ~(34)S_(v-CDT)=-27.46‰,经历了强烈的有机地质作用;铀石围绕炭屑、星散状黄铁矿产出,被胶状黄铁矿肢解,铀富集于成岩作用后期。由此认为,直罗组同生沉积过程中预富集的铀为主要成矿铀源,东胜铀矿田属直罗组预富铀重新分配的产物。 相似文献
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东胜地区砂岩型铀矿成矿年代学及成矿铀源研究 总被引：15，自引：0，他引：15
文章研究了鄂尔多斯盆地东胜地区砂岩型铀矿成矿年代学特征。东段铀矿体翼部的成矿年龄为120±11 Ma和80±5 Ma,矿体卷头部位的成矿年龄为20±2 Ma、8±1 Ma;中段有124±6Ma和80±5 Ma的成矿年龄。这表明早白垩世和晚白垩世是该区铀的主成矿期,它与盆地抬升的构造演化历史相一致。卷头(富矿)铀成矿作用发生在新近纪中新世和上新世,可能与该时期区内的构造热事件有关。新近纪铀的成矿作用对早期铀矿化起到改造作用。铀含量<0.01%的样品U-Pb等时线年龄为177±16 Ma,在误差范围内与直罗组的沉积年龄(中侏罗世)相吻合,这是直罗组沉积时铀预富集的直接证据。砂体原始含量(U0)的研究结果显示,U0平均值为24.64×106,也表明有铀的预富集。直罗组岩石中铀的近代得失(ΔU)研究结果表明,其ΔU的平均值为70.2%,显示非矿化岩石以带出铀为主,是铀成矿的重要铀源。 相似文献
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新华地区作为鄂尔多斯盆地南部中侏罗统直罗组找矿的重点地区之一,研究其沉积特征及铀成矿条件对指导该区砂岩型铀矿勘查工作至关重要。文章通过岩心观察及钻孔资料综合分析,编制了直罗组地层厚度、砂体厚度、含砂率、氧化率等值线图等系列图件,对直罗组沉积相及铀成矿条件进行了综合分析。结果表明：新华地区直罗组上段主要发育曲流河相沉积,可分为曲流河河道、边滩、天然堤以及河漫滩微相沉积,直罗组下段以辫状河相沉积为主,可分为辫状河河道、心滩、泛滥平原微相沉积,其中,直罗组下段辫状河河道砂体厚度适中,连通性好,富含还原物质,是有利的成矿相带。新华地区构造发育,存在构造天窗,层间氧化带发育,直罗组下段辫状河河道呈南北向展布,氧化带与砂体展布基本一致,具有有利的铀成矿条件。综合构造条件、沉积特征、后生蚀变特征和铀矿化信息,结合煤田自然伽马异常,认为研究区西北部店头赵村—白店—崔家岭一带是铀成矿最有利区域,可以作为直罗组砂岩型铀矿下一步勘查的重点目标区。 相似文献
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《古地理学报》2020,(2)
鄂尔多斯盆地南部中侏罗统直罗组下段砂岩中已发现店头砂岩型铀矿床及多个铀矿点,但对于盆地南部直罗组沉积相研究较为薄弱,制约了砂岩型铀矿的进一步找矿工作。通过剖面实测、岩心编录,结合石油、煤炭、核工业地质钻孔资料,对鄂尔多斯盆地南部直罗—店头地区直罗组沉积特征进行精细刻画。在此基础上,探讨了沉积相与铀成矿的关系及下一步找矿方向。结果显示,直罗组下段砂体厚度30～65 m、砂地比在0. 6～0. 75之间,为砂质辫状河沉积。直罗组上段早期砂体厚度10～38 m、砂地比值在0. 15～0. 45之间,为曲流河沉积;直罗组上段沉积晚期研究区位于湖盆中心所在位置,为滨浅湖沉积。沉积环境、沉积相、辫状河河道交汇部位、砂体厚度、沉积物粒度及泥岩夹层对铀成矿具有重要控制作用。直罗组下段辫状河河道交汇或分叉部位应作为勘查重点,心滩亚相的含炭屑、黄铁矿砂质碎屑岩可作为铀矿化的找矿标志。 相似文献
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为了明确黄陵地区中生代含煤岩系油气与铀成矿的耦合关系,进行了钻孔与剖面的野外地质调查、钻孔资料与实验数据的分析与处理、油气藏与铀矿（点）信息的综合整理,系统研究了中生代含煤岩系构造–沉积体系、铀矿地质特征和油气地质特征,从油气藏与铀矿（点）的空间分布关系、含烃流体与铀的伴生蚀变矿物的成因关系以及烃源岩生烃与铀成矿的时间关系展开讨论。研究表明:中生代含煤岩系铀矿（点）多分布在基岩剥蚀边界或小型断裂附近,且水平投影位于油气有利相带周缘;烃类流体组分及煤层气的中间产物可能参与氧化还原反应,生成黄铁矿、方解石等与铀矿物具有密切伴生关系的矿物;中生代含煤岩系烃源岩主生烃期和排烃期总体早于铀矿主成矿期,烃类流体可能通过运移影响铀成矿作用。 相似文献
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准噶尔盆地南缘硫磺沟地区铀矿化砂岩流体包裹体及有机地球化学特征 总被引：1，自引：0，他引：1
准噶尔盆地南缘硫磺沟地区伴随铀矿化发育较多地沥青、油气残留物。为查明两者间的关联性,对含地沥青铀矿化砂岩进行了流体包裹体测试和有机地球化学分析。镜下观察发现,包裹体以含烃盐水包裹体和液烃包裹体为主,少量气烃包裹体。测温结果表明,含烃盐水包裹体均一温度及盐度整体中等偏低,分别集中于60~90℃、0%~8%NaCl。结合GOI统计及酸解烃测试结果得出含矿砂体主要存在一期中等偏弱的油气充注。气相色谱-质谱分析得出:主峰碳为C_(14)~C_(25),单峰型;OEP与CPI分别为0.474~1.58、0.887~2.70,分布较分散;Pr/Ph为0.40~1.43,多小于1;Pr/nC_(17)、Ph/nC_(18)分别为0.164~0.833、0.595~1.54,质量色谱图基线"鼓包"不明显。以上表明油气有机质来源以低等藻类为主,总体处于较强还原环境,成熟度差异较大,生物降解微弱。基于油气还原与铀成矿间的关系及野外地质特征,认为油气还原对本区铀成矿有两大作用:一是对下中侏罗纪的早期铀矿体起保矿及隐蔽作用;二是进一步提高上侏罗统砂岩层的还原容量,为后期铀成矿提供所必需的还原场。 相似文献
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Guboglo M. N. 《GeoJournal》1980,4(1):53-58
International unity is becoming ever stronger in this country owing to an increasing similarity in the development of the cultural environment. This comprises the provision of all the country's republics with a sufficient number of schools, theatres, and other institutions and cultural information media in accordance with the needs of the population. An important part is played by the rise in ‘the general educational level, as well as the level of professional qualifications and skills. Among all the Soviet nations and nationalities, this rise being more rapid among formerly backward peoples. Prominent among the factors of internationalization is the progressive development of the nationalities’ cultural resources, while professional culture is being increasingly brought within the reach of the masses.The implementation of the nationalities policy promotes the all-round development of all Soviet nations and nationalities, their drawing together, the upsurge of the individual capabilities of every Soviet citizen. 相似文献
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Deviation of the major axis of the inertia ellipsoid of the Moon from the direction toward the Earth
B. P. Kondratyev 《Astronomy Reports》2017,61(8):709-714
It is known from observations that the center of mass of the Moon does not coincide with the geometric center of its figure, and the line connecting these two centers is not aligned with the direction toward the center of the Earth, instead deviating toward the Southeast. This stationary deviation of the axis of the inertia ellipsoid of the Moon to the South of the direction toward the Earth is analyzed. A system of five linear differential equations describing the physical libration of the Moon in latitude is considered, and these equations are derived using a new vector method taking into account perturbations from the Earth and partly from the Sun. The characteristic equation of this system is obtained, and all five oscillation frequencies are found. Special attention is paid to the fifth (zero) frequency, for which the solution of the latitude libration equations are stationary and represents a previously unknown additional motion of the rotational axis of theMoon in a cone with a small opening angle. In contrast to the astronomical precession of the Earth, the rotation of the angular-velocity vector is in the positive direction (counter-clockwise), with the period T 3 = 27.32 days. On this basis, this phenomenon has been named “quasi-precession.” This quasi-precession leads to a stationary inclination of the major axis of the inertia ellipsoid of theMoon to the South (for an observer on Earth), making it possible to explain one component of the observed deviation of the center of mass of the Moon from the direction toward the Earth. The opening angle of the quasiprecession cone is approximately 0.834″. 相似文献
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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. 相似文献
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摩擦桩基桩土间极限摩阻力取值问题探讨 总被引：1，自引：0，他引：1
通过对广珠东线高速公路横沥大桥的试桩及土体的工程地质条件分析,总结出影响摩擦桩基桩土间极限摩阻力取值的一般问题以及解决问题的方法和措施。 相似文献
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位于华北和扬子两板块碰撞带中的苏鲁榴辉岩形成的温压条件不但是超高压，而且是高温。榴辉岩的PTt轨迹表明其为陆-陆磁撞俯冲带的产物。榴辉岩的区域性围岩花岗质片麻岩为新元古代同碰撞期花岗岩，榴辉岩及其他直接围岩皆呈包体存在于其中，并见新元古代花岗岩呈脉状侵入榴辉岩包体中。区域性围岩新元古代花岗岩的锆石中发现有柯石英、绿辉石等包裹体，表明新元古代花岗岩的组成物质也经受过超高压变质作用，且榴辉岩与围岩新元古代花岗岩的锆石U-Pb体系同位素年龄基本相同。但新元古代花岗岩所记录的变质作用和变形作用期次（或阶段）却少于榴辉岩。椐上述可得如下推断：超高压榴辉岩与新元古代花岗岩岩浆是同时在碰撞带底部（俯冲板块前部）形成的；榴辉岩的第一折返阶段是由新元古代花岗岩岩浆携带上升的，其第二折返阶段是和新元古代花岗岩一起由逆冲及区域性隆起而上升，遭受剥蚀。 相似文献
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某高速公路下伏煤矿采空区稳定性分析 总被引：10，自引：0，他引：10
在论述某高速公路下伏砦脖煤矿采空区地质、采矿和工程地质特征的基础上, 进行了稳定性数值模拟分析, 定性与定量地分析与评价了该煤矿采空区的地表变形特征及稳定性。研究结果表明: 该煤矿采空区的变形尚未完成, 对拟建的高速公路将产生很大的危害, 必须采取相应的工程治理措施。 相似文献
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The Importance of the Precipitation and the Susceptibility of the Slopes for the Triggering of Landslides Along the Roads 总被引：3，自引：1，他引：2
Clemente Irigaray Francisco Lamas Rachid El Hamdouni Tomás Fernández José Chacón 《Natural Hazards》2000,21(1):65-81
In order to characterise the influence of the heavyrains on the observed landslides during the 1996–1997hydrological cycle, rainfall records for the last 100years are analysed from 104 stations in easternAndalusia. Regarding the amounts of rain recordedbetween October 1996 and March 1997 in the 104stations studied, 31 presented new all-time records;15 presented values that were 80–100% of thepre-1995 record; 49 stations, 80–50%; and 9stations, < 50%. A map has been devised of thesusceptibility of the materials through which thesouth-eastern Andalusian road network crosses,together with an inventory of the damage caused byinstability phenomena on banks and cuttings of theroad network during the winter of 1996–1997. Therelationships between the rainfall during the studyperiod, the damage caused to the road network and thesusceptibility of the materials affected are analysed.The results indicate that there is a clearcorrespondence between the rainfall recorded and thesusceptibility of the materials with the inventorieddamage. It is concluded that the widespread seriousdamage caused in early 1997 to the roads andsurrounding areas in the Alpujarra region and thecoast of the Province of Granada was mainly caused bythe extraordinarily heavy rains. However, considerablyless damage was observed where the susceptibility ofthe terrain is low, thus highlighting the extremeusefulness of terrain-susceptibility maps for riskprevention and territorial planning. 相似文献
20.
The structure of the eastern Pyrenees consists mainly of south-directed thrusts involving basement and cover rocks. An antiformal stack developed by the piling up of basement thrust sheets which outcrop in the Axial zone. These structures account for a thin-skinned thrust model rather than a vertical fault model in which the Axial zone would be essentially autochthonous, and the North-Pyrenean fault the axial plane of a fan thrust system. New data from the Eastern Pyrenees and the thin-skinned model suggest that(1) the structure east of the Pedraforca nappe is similar to that of the Central Pyrenees; (2) the cover rocks of the South-Pyrenean units and of the Axial zone-after restoration—built up a northwards-thickening prism consistent with the existence of a unique Pyrenean sedimentary basin during Mesozoic time; (3) the Axial zone is only a complex antiformal stack developed as a part of South-Pyrenean system related to the Paleogene thrusting-tectonics. The Axial zone palaeogeographic area had no special meaning during Mesozoic time. 相似文献