华北南缘中元古界高山河群碎屑锆石U-Pb年代学及其地质意义

为了探讨华北板块南缘中元古代沉积地层的时代归属和物质来源、区域古地理格局和大地构造特征,对豫西灵宝福地地区的高山河群进行碎屑锆石U-Pb年代学和锆石微量元素特征研究。获得的高山河群年龄最小(年轻)的单颗碎屑锆石207Pb/206Pb年龄值为1685±39 Ma,从而限制了高山河群最早沉积年龄不早于1700 Ma。结合上覆的龙家园组年代学标定(1594±12 Ma),将高山河群的形成年代限定为1700—1600 Ma,即中元古代长城纪的中晚期,属国际地质年表的"固结纪"。高山河群中碎屑锆石207Pb/206Pb年龄范围为1685—2751 Ma,呈现1850 Ma、2150 Ma、2300 Ma和2500 Ma共4个年龄峰值,对应于华北克拉通古元古代重要的地质事件,并且高山河群以1850 Ma和2500 Ma峰值年龄段的地质体为主要的物源区。根据高山河群与云梦山组碎屑锆石年龄频率对比,推测在豫西地区西侧存在以往报道较少的年龄为2500 Ma的地质体。根据熊耳群火山岩及其对应锆石的地球化学特征和熊耳期盆地动力学性质,并结合高山河群沉积相特征和沉积盆地构造属性,认为熊耳群形成于与"岛弧"共生的拉张性质的弧后盆地地区,而其上覆的高山河群为弧后盆地靠近大陆一侧的具有被动大陆边缘性质的滨浅海沉积。     

华北南缘中元古界高山河群碎屑锆石U-Pb年代学及其地质意义*

为了探讨华北板块南缘中元古代沉积地层的时代归属和物质来源、区域古地理格局和大地构造特征,对豫西灵宝福地地区的高山河群进行碎屑锆石U-Pb年代学和锆石微量元素特征研究。获得的高山河群年龄最小(年轻)的单颗碎屑锆石 ²⁰⁷Pb/²⁰⁶Pb 年龄值为1685±39 Ma,从而限制了高山河群最早沉积年龄不早于1700 Ma。结合上覆的龙家园组年代学标定(1594±12 Ma),将高山河群的形成年代限定为1700—1600 Ma,即中元古代长城纪的中晚期,属国际地质年表的“固结纪”。高山河群中碎屑锆石 ²⁰⁷Pb/²⁰⁶Pb 年龄范围为1685—2751 Ma,呈现1850 Ma、2150 Ma、2300 Ma和2500 Ma共4个年龄峰值,对应于华北克拉通古元古代重要的地质事件,并且高山河群以1850 Ma和2500 Ma峰值年龄段的地质体为主要的物源区。根据高山河群与云梦山组碎屑锆石年龄频率对比,推测在豫西地区西侧存在以往报道较少的年龄为2500 Ma的地质体。根据熊耳群火山岩及其对应锆石的地球化学特征和熊耳期盆地动力学性质,并结合高山河群沉积相特征和沉积盆地构造属性,认为熊耳群形成于与“岛弧”共生的拉张性质的弧后盆地地区,而其上覆的高山河群为弧后盆地靠近大陆一侧的具有被动大陆边缘性质的滨浅海沉积。     

豫西汝阳群、洛峪群碎屑锆石年代学特征及其地质意义

华北克拉通南缘"豫陕裂陷槽"发育大量中—新元古代地层,其中汝阳群和洛峪群分布于渑池—确山地层小区,其形成时代一直存有争议.本文针对汝阳群和洛峪群沉积岩进行了系统的碎屑锆石年代学研究工作,结合地层发育和岩石组合分析,为建立华北克拉通南缘中—新元古代地层框架提供依据.根据云梦山组下部碎屑锆石中获得年轻锆石年龄平均值1723.6 Ma,结合前人从洛峪群凝灰岩夹层中获得的年代学资料(1611±8 Ma、1640±16 Ma、1638±9 Ma、1634±10 Ma),将汝阳群-洛峪群的沉积时限限定在1720～1600 Ma之间.本文所采集的云梦山组、白草坪组和崔庄组样品中碎屑锆石207Pb/206Pb年龄分别在2657～1739 Ma、2712～1780 Ma和2654～1819 Ma之间,说明三个组沉积物质主要来源于古元古代地质体,部分为新太古代地质体.鲁山地区发育的新太古代—古元古代的太华杂岩,登封地区发育的新太古代登封群以及古元古代嵩山群和花岗质岩石等,均可为中—新元古代沉积岩提供物源.豫西地区汝阳群-洛峪群碎屑锆石中～2.7 Ga、～2.5 Ga、2.1～2.0 Ga和1.85～1.8 Ga的年龄谱峰值分别对应华北克拉通早前寒武纪发生地壳生长、克拉通化、裂谷和造山等重要地质事件.越来越多资料显示华北克拉通在2.2～2.0Ga时期存在强烈的岩浆活动,豫西地区～2.1 Ga的岩浆作用也逐渐被识别出来.     

燕山地区团山子组层凝灰岩SHRIMP锆石U-Pb年龄及其地质意义

燕辽地区长城群年代学工作一直是华北克拉通中元古代地质学研究的重点之一。由于团山子组与下伏串岭沟组界限年龄不明确,且此前的年龄都是来自于其中的火山熔岩锆石的年龄,亟待新的测年工作加以验证和完善。本文作者在北京市密云区、平谷区的团山子组下部发现了层凝灰岩,并对其开展了系统的SHRIMP锆石U-Pb测年,获得两个高精度年龄1634±9Ma和1637±8Ma,进一步精确限定了该组的形成年代。结合前人研究,燕辽地区团山子组的底界、也即下伏串岭沟组顶界年龄,可进一步限定为1638Ma。由此可对燕辽地区长城群地层格架进行更准确的年代学厘定,并进一步确认其整体处于持续拉张的裂谷-被动陆缘背景下的快速沉积特征、以及长城群团山子组-大红峪组与华北克拉通南缘汝阳群洛峪口组等相关沉积更为精确的对比关系。结合其他资料还可推断,在团山子组-大红峪组及洛峪口组等形成时,华北克拉通南北两侧都开始被碳酸盐岩浅海覆盖,且最终还可能在其中部出现了南北联通的碳酸盐岩浅海通道。这显示出华北克拉通与早先所拼合克拉通之间已产生明显的拉张性疏离及新生海洋,应标志着华北克拉通从哥伦比亚超大陆裂解的新阶段。     

东阿拉善地块诺尔公群石英岩的碎屑锆石年龄特征——物源区制约及其地质意义

传统上将阿拉善地块东部变质基底"阿拉善岩群"之上的一套以石英岩、浅粒岩、碳酸盐岩及碎屑岩为主的浅变质地层称为诺尔公群,并根据区域地层对比及叠层石化石将其归为"长城纪"。为进一步限定地层时代,对诺尔公群底部3件石英岩进行LA-MC-ICP-MS锆石U-Pb测年,获得的年龄主要集中在2 530~2 500 Ma和1 950~1 850 Ma两个年龄段内,另外还获得少量年龄为~1.69 Ga、~2.0 Ga、~2.15 Ga、~2.35 Ga、~2.7 Ga和~3.4 Ga的锆石。其中,最年轻的碎屑锆石年龄限定了诺尔公群底部石英岩的沉积时代晚于1.69 Ga,结合上覆地层的年龄数据将诺尔公群的沉积时代大致限定为1.69~1.29 Ga,肯定了阿拉善地块存在中元古代地层。石英岩中~2.5 Ga和~1.95 Ga两个显著的碎屑锆石年龄峰符合典型的华北克拉通物源区特征,因此认为,阿拉善地块在太古代-中元古代具有与华北克拉通相似的构造环境,是华北克拉通的一部分。     

华北克拉通西南缘汝阳群沉积时代及其地质意义：来自碎屑锆石U-Pb年龄的证据

汝阳群分布在华北克拉通西南缘,位于河南-陕西-山西交界地区,主要为一套未变质的碎屑岩及碳酸盐岩地层,不整合于熊耳群火山岩系之上,其上被洛峪群整合覆盖。长期以来,其地质时代一直存有较大的争议。本文通过对汝阳群下部白草坪组4个石英砂岩样品中的碎屑锆石进行LA-ICP-MS U-Pb年龄测定,获得的²⁰⁷Pb/²⁰⁶Pb年龄分布范围为3 000～1 800 Ma,主要集中在2 600～2 400 Ma之间(约占67%),年龄主峰值为2 550～2 500 Ma,说明其沉积物质主要来源于新太古代末以及古元古代的地质体。其中,最年轻锆石的²⁰⁷Pb/²⁰⁶Pb谐和年龄值分别为1 817±22 Ma、1 838±23 Ma、1 924±17 Ma和1 829±28 Ma,说明汝阳群沉积时代不老于1 800 Ma,与其上覆洛峪群中近期获得1 611±8 Ma的年龄相吻合,因此其形成时代应为中元古代早期。     

天津蓟州东水厂中元古代高于庄组凝灰岩锆石SHRIMP U-Pb年龄 ——对中元古代生物-环境事件的制约

对华北克拉通北缘中-新元古界标准剖面的高于庄组第三亚组(张家峪亚组)下部凝灰岩样品进行了锆石SHRIMP U-Pb定年,获得~(207)Pb/~(206)Pb加权平均年龄1 582±12 Ma。该凝灰岩层厚度约15 cm,层位介于高于庄组第三亚组下部"瘤状灰岩"层与含宏观藻类化石(Parachuaria glabra.)层之间,紧邻藻类化石层。该地层时代为高于庄组属于国际中元古界盖层系(Calymmian System)下部层位提供了新依据,为中元古代高于庄组全球生物-环境事件及全球对比提供了重要约束。     

华北克拉通南缘官道口群和洛峪群的年代学研究新进展——来自凝灰岩SHRIMP锆石U-Pb年龄的新证据

华北克拉通南缘结晶基底之上广泛发育中-新元古代(1800～542Ma)盖层岩系,但由于缺少精确的同位素年龄数据,其地层划分和对比方案一直存在较大的争议。本次工作在河南省栾川县龙家园组底部和下部各发现了一套凝灰岩,进而获得了1594±12Ma和1541±8Ma的SHRIMP锆石U-Pb年龄,首次精确标定了该地区龙家园组的形成时限,该组底界的时代接近1600Ma。龙家园组沉积时代为中元古代蓟县纪最早期;在河南省汝阳、汝州、鲁山地区的洛峪口组凝灰岩中获得了1596±7Ma、1596±15Ma、1608±17Ma和1620±16Ma的SHRIMP锆石U-Pb年龄,进一步精确标定了洛峪口组的形成时代,洛峪口组形成于长城纪的末期。结合汝阳群云梦山组碎屑锆石U-Pb年龄结果,汝阳群-洛峪群的形成时限约为1700～1600Ma。官道口群应是汝阳群之后的地层系统,而不是早前认为的与之同期的地层。     

华北串岭沟组凝灰岩锆石SHRIMP年龄及其地层学意义

华北克拉通燕辽地区是中国中新元古代沉积地层的标准剖面区。蓟县群和青白口群已经取得了很多重要的高精度定年数据,但是长城群除了顶部大红峪组有了高精度定年以外,其他组还缺乏可靠的高精度定年数据。为了准确标定华北克拉通中元古界长城群串岭沟组的年龄,对采自河北宽城地区神仙岭剖面串岭沟组顶部火山岩凝灰岩锆石进行了SHRIMP U-Pb定年。结果表明所测锆石207Pb/206Pb表面年龄加权平均值为(1 634.8±6.9) Ma(95% 置信度,MSWD=1.2,n=23)。可见长城群串岭沟组顶部的准确年龄为(1 634.8±6.9) Ma,表明长城群串岭沟组到大红峪组整体上属于中元古代地层。     

华北陆块东北缘张三沟岩组SHRIMP锆石U－Pb年代学研究及其地质意义

出露于华北陆块东北缘的张三沟岩组为一套变质火山－沉积岩系,前人根据变质程度和地层对比将其划归古元古代。本文通过SHRIMP锆石U-Pb年代学研究,获得2517±9 Ma 、2518±7 Ma 和2534±26Ma原岩年龄,2439±24Ma、2464±73Ma和2433±71Ma变质年龄。这表明该套变质岩层形成于新太古代晚期,变质时代在新太古代末－古元古代初。结合区域资料,其变质年龄可能代表了古龙岗陆块与位于其北东侧的其它陆块（如佳木斯陆块）碰撞造山的时代,表明华北克拉通在新太古代末－古元古代初期经历过一次重要的克拉通化。     

东濮凹陷北部沙河街组三段中亚段沉积环境分析

东濮凹陷北部沙三中亚段广泛发育盐岩和烃源岩,这两个看似不能共存的物质却在这里互层共生。该时期研究区沉积特征为多盐韵律与多层烃源岩互层共生、连续沉积,单个盐韵律厚度从几米到十几米,烃源岩有机质丰度高、类型好。平面上,两者在湖盆沉积沉降中心共生;垂向上,高有机质丰度、好干酪根类型与高盐度地层具有较好的对应关系。因而成为恢复古气候和古环境的重要研究对象。通过岩石学、古生物学以及Sr/Ba、B/Ga、(V+Ni+Mn)、Fe/Mn、Sr/Cu、Mg/Ca、V/(V+Ni)、稀土元素含量和氯同位素等方法对凹陷北部沙三中亚段的沉积环境进行研究。结果表明,凹陷北部沙三中亚段为深水沉积的还原环境,古盐度较高,达到半咸水-咸水沉积;微量元素和孢粉化石特征表明研究区沙三中亚段为温暖潮湿的环境。     

The Importance of the Precipitation and the Susceptibility of the Slopes for the Triggering of Landslides Along the Roads

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.     

郯庐断裂南段研究进展与断裂性质讨论

据1：5万区域地质调查和专题研究资料，就郯庐断裂带是否南延与消失的原因，其与大别—苏鲁造山带交截形成的假位错效应，以及与中新生代沉积盆地形成演化的关系等作了新的阐述。在此基础上，讨论了郯庐断裂带是否为巨大的左行平移断层或转换断层。认为郯庐断裂带可能是在“古郯庐带”的基础上于早侏罗世重新活动、白垩纪强烈活动的地堑型枢纽断裂带。     

塘口水电站坝基岩体透水性和渗漏问题分析

塘口水电站大坝基础座落在断层和裂隙较发育的龟裂纹灰岩上,岩体完整性差、透水性强,多年运行后,大坝灌浆廊道和排水廊道出现多处集中性漏水,为确保大坝安全和电站正常发电,根据渗漏性质和成因,采用对灌浆廊道补充帷幕灌浆,对排水廊道进行固结+帷幕+回填灌浆。通过灌浆处理后,效果良好,表明灌浆工程有效的将导致坝基渗漏的上下游的裂隙通道封闭,并顺利的经受了随后的汛期洪水考验,大坝安全得到保障。     

Unity of the national and the international in the socio-cultural development of the peoples of the USSR

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.     

某高速公路下伏煤矿采空区稳定性分析

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。      

Report of the restudy of the defined global stratotype of the base of the Silurian System

The Global Stratotype Section and Point （GSSP） for the base of the Silurian System was defined in 1985. Since that time, a number of researchers have suggested that this section has serious deficiencies for use as a GSSP. As a result, in 2000, the Subcommission on Silurian Stratigraphy （SSS） proposed undertaking a formal restu@ of this GSSP, which was subsequently approved by the International Commission of Stratigraphy （ICS）. The result of this restudy was the formal proposal that the current GSSP, at 1.6 m above the base of the Birkhill Shale, at Dob＇s Linn, Scotland, should be maintained as the same locality and stratigraphic level, but the bios- tratigraphical definition of the boundary should be revised. The previously defined, basal Silurian grapto- lite zone, the Parakidograptus acuminatus Zone, should be subdivided into a lower Akidograptus ascensus Zone and a higher E acuminatus Zone. The base of the A. ascensus Zone, marked by the first appearance of A. ascensus, should be regarded as the biostratigraphic mark for the base of the Silurian. This proposal has now been formally approved by the SSS and ICS, and ratified by International Union of Geological Sciences. This is the first GSSP to undergo formal restudy and redefini- tion, and the proposal also included a recommended procedure for restudy of GSSPs.     

Calculation of the Inverse of the Covariance

In reservoir characterization, the covariance is often used to describe the spatial correlation and variation in rock properties or the uncertainty in rock properties. The inverse of the covariance, on the other hand, is seldom discussed in geostatistics. In this paper, I show that the inverse is required for simulation and estimation of Gaussian random fields, and that it can be identified with the differential operator in regularized inverse theory. Unfortunately, because the covariance matrix for parameters in reservoir models can be extremely large, calculation of the inverse can be a problem. In this paper, I discuss four methods of calculating the inverse of the covariance, two of which are analytical, and two of which are purely numerical. By taking advantage of the assumed stationarity of the covariance, none of the methods require inversion of the full covariance matrix.     

Deviation of the major axis of the inertia ellipsoid of the Moon from the direction toward the Earth

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″.