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1.
西藏班戈县保吉地区各昌茶玉剖面发现晚侏罗世珊瑚化石约12属16种,分别为Calamophylliopsis?sp.,Clausastraea?sp.,Epistreptophyllum cylindratum Milaschevitsch,Epistreptophyllum sp.,Heliocoenia aff.etalloni Koby,Kobyastraea?sp.,Montlivaltia tenuilamellats Roniewicz,Montlivaltia?sp.,Myriophyllia?sp.,Pseudocoenia hexaphyllia(d’Orbigny),Pseudocoenia?sp.,Rhipidogyra?sp.,Stephanastraea?sp.,Stylina?sp.,Stylina cf.subramosa de Fromentel,Thecosmilia?sp.等。化石指示各昌茶玉剖面上部第42—80层时代为晚侏罗世牛津期—基默里奇期,表明各昌茶玉剖面地层并不属于原划的中二叠统下拉组。本文依据化石及岩性特点将其修订为上侏罗统吐卡日组。根据保吉地区的吐卡日组与上下地层的接触关系及其岩性变化可划分为上下两段地层,各昌茶玉剖面代表吐卡日组下段地层,主要为厚层碳酸盐岩夹少量泥页岩及多层礁灰岩。久朗仓剖面代表吐卡日组上段地层,为一套碳酸盐岩夹大量粗碎屑岩地层。吐卡日组下段在措勤盆地内部、班公湖—怒江缝合带内广泛分布,指示晚侏罗世措勤盆地发育大面积广阔稳定的碳酸盐岩台地,其中生物礁表明晚侏罗世碳酸盐岩台地具有优越的油气生成和储集条件。 相似文献
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措勤盆地东部班戈县保吉乡各昌茶玉地区发现晚侏罗世珊瑚化石约10属15种及未定种,分别为Actinaraea?sp.,Allocoenia?sp.,A.matheyi(Koby),Clausastraea?sp.,Hydnophora?sp.,Latiastraea minima(Koby),Latiastraea?sp.,Meandraraea?sp.,Stylosmilia crassitheca Liao et al Li,S.corallina Koby,Thamnasteria?sp.,T.concinna(Goldfuss),Thecosmilia.baojiensis sp.nov.,Thecosmilia?sp.,Trocharaea cf.patelliformis Gregory等。化石指示各昌茶玉剖面第1—41层地层时代为晚侏罗世牛津期—基默里奇期。珊瑚化石产出的层位原来被认为是混杂在中侏罗世蛇绿岩中的中二叠统下拉组,本文根据剖面中化石及岩性组合特点将其修订为上侏罗统萨波直不勒组,并得出了该地区不存在原来所认为的中二叠统下拉组与中侏罗统蛇绿岩构造混杂现象的认识。本次萨波直不勒组与改则县物玛乡抢古村建组剖面相对比,其岩性更细、灰岩夹层更多,珊瑚化石更为丰富,代表了更远离陆源碎屑源区的沉积环境,进一步证明晚侏罗世冈底斯地区地势是从北向南逐渐加深的,措勤盆地在晚侏罗世处于活动型深海-半深海相和上斜坡相的沉积环境中。保吉地区萨波直不勒组顶部存在上斜坡相68 m厚黑色泥页岩,TOC(总有机碳)平均值为0.83%,属于中等-好烃源岩,剖面第20层12 m厚黑色泥岩TOC值为0.65%,属于中等烃源岩。萨波直不勒组顶部为上斜坡相沉积,分布范围应该比上覆的吐卡日组更广泛。经计算,措勤盆地内萨波直不勒组烃源岩的生烃量约为44.373亿吨。萨波直不勒组的泥页岩为措勤盆地提供了充足的油源保障,同时其中的碳酸盐岩夹层也可能是油气有利储层,建议对上侏罗统萨波直不勒组开展钻探取样工作,获取更为翔实丰富的有机地球化学参数。 相似文献
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西藏班戈县扎穷地区古生界混杂岩块中发现中生代化石 总被引：1，自引：0，他引：1
西藏班戈县新吉乡扎穷地区新发现了晚侏罗世珊瑚化石10属11种:Stylina?sp.、Goniocora annulata Roniewicz,Epistreptophyllum cf.cornutiformis(Gregory),Solenocoenia?sp.,Calamophylliopsis moreauana(Michelin),Thamnasteria?sp.,Clausastraea?sp.、Isastraea?sp.,Montlivaltia?sp.,Montlivaltia tenuilamellata Roniewicz,Thecosmilia?sp.,早白垩世珊瑚化石3属3种:Eohydnophora tosaensis YabeEquchi、Clausastraea tabulate Morycowa、Stylosmilia baojiensis sp.nov.,早白垩世腹足类化石5属8种:Mesoglauconia neumayri(Nagao),Rhabdocolpus asiaticum Djalilov,Pseudomesalia bangoinensis Yu,Mesoglauconia bicarinata(Hamlin),Mesoglauconia arkelli Mennessier,Nerinea domaensis Yu,Mesoglauconia cf.arkelli Mennessier,Microschizacf.inflata Orbigny。根据上述化石,原中二叠统下拉组被修订为上侏罗统吐卡日组和下白垩统朗山组,原下石炭统永珠组被修订为下白垩统多尼组。上述地层时代修订的意义如下:(1)上侏罗统吐卡日组的分布范围向南可以到达扎穷地区,进一步否定了冈底斯南部在晚侏罗世是古陆的认识。(2)朗山组和多尼组的发现指示早白垩世海相地层分布范围向南可以扩展到扎穷地区,这对冈底斯南部在早白垩世是古陆或岛弧的认识提出了质疑。(3)扎穷地区不存在古生界岩块与中侏罗统蛇绿岩构造混杂的现象。本区的构造活动强度并不强烈,没有造成古生界岩块大规模出露并混杂堆积的现象。(4)因为吐卡日组、多尼组和朗山组分布范围的扩大、措勤盆地中部构造破坏并不强烈,所以措勤盆地的油气前景进一步变好。 相似文献
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在西藏措勤断块新建了中三叠统—上三叠统卡尼阶岩石地层单位——嘎热扎地组。在建组剖面上,嘎热扎地组厚约485 m,下部岩性以碎屑岩为主上部岩性为碎屑岩夹灰岩。嘎热扎地组与下伏上二叠统—下三叠统木纠错组、上覆上三叠统诺利阶麦龙岗组均为整合接触关系。该组尚未发现指示地层时代的化石,但前人在其下伏的木纠错组中发现了早三叠世牙形石本次在其上覆的麦龙岗组发现7属8种珊瑚化石:Distichophyllia norica(Frech),Retiophyllia?sp.,Cablonzeria?sp.Elysastraea juliana Turnsek,Volzeiasublaevis (Munster),Distuhophyllia sp.,Guembelastraea?sp.和Benedcastraea baiyuensis Deng&Zhang。根据该组地层整合于两者之间,将其时代暂时限定为中—晚三叠世卡尼期。根据珊瑚化石、地层岩性特征及上下地层关系将研究剖面的地层进行了重新划分。嘎热扎地组的建立填补了措勤断块局限台地相三叠系序列中三叠统—上三叠统卡尼阶岩石地层单位名称的空白。嘎热扎地组建立以后,措勤断块局限台地相三叠系的岩石地层单位序列可以划分为上二叠统—下三叠统木纠错组,中三叠统—上三叠统卡尼阶嘎热扎地组,上三叠统诺利阶麦龙岗组,上三叠统瑞替阶—下侏罗统确哈拉组。这一序列的建立对于在措勤断块进一步识别出碳酸盐岩局限台地相三叠系,修订相关地区的地层认识具有指导作用。 相似文献
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在西藏羌塘盆地昂达尔错地区前人划分的上三叠统角木日茶卡组中发现了二叠纪化石分子Acanthopecten cf.coloradoensis(Newbrry)和Pterinopectinella?sp.,结合岩石组合特征,经过进一步开展生物年代对比及区域地层对比,将该套角木日茶卡组重新厘定为中二叠统龙格组,从而首次将羌塘盆地东南侧出露地层的时代下限由原来的上三叠统修正至中二叠统,增添了新的古生物化石证据。首次明确了中央隆起带东段的南羌塘地区中新生代之下存在晚古生代地层,为今后更深入研究羌塘盆地零星出露的古生代地层及地质演化提供了重要基础资料。 相似文献
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实测西藏改则县甲不拉东剖面过程中,在前人原划分为二叠系下拉组中采集到属于晚侏罗世时代的生物化石(Microso lena sp.Meandronhyllia、Thecosmilia sp.Burgundia sp.Buneia sp.),根据岩石组合及生物化石面貌等区域地层对比,将该套地层确定为上侏罗统吐卡日组。该套地层的确定,为班公湖-怒江结合带侏罗纪珊瑚动物群的研究、洋盆的萎缩、消亡及洋-陆转化提供新的基础地质资料。 相似文献
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在西藏措勤打加错地区新发现上三叠统江让组,其为一套海相碎屑岩及碳酸盐岩沉积建造,岩性主要为不等厚层状石英质砾岩、深灰色薄层状—块状生物碎屑微晶灰岩、含砂粉砂质微晶灰岩、含石英砾质生物碎屑灰岩、砂屑灰岩夹钙质细砂岩,产珊瑚Distichophyllia sp.,Volzeia sp.,Montlivaltia sp.,M.cf.xainzaensis、海绵:Hartmanina sp.和双壳类Xenocardita?sp.,时代为晚三叠世卡尼期-诺利期,与下二叠统昂杰组呈角度不整合接触。江让组在该地区的发现,完善了冈底斯西部三叠纪的地层系统,为研究印支运动对冈底斯西部的影响和古特提斯洋的演化提供了依据。 相似文献
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内蒙古西部北山地区甜水井-青山一带双堡塘组时代讨论 总被引：3，自引：2，他引：3
通过对神螺滩双堡塘组生物地层的研究、对比,神螺滩双堡塘组中所产菊石Uraloceras是北山地区双堡塘组的特征分子,广泛分布于俄罗斯、加拿大、澳大利亚和中国的上石炭统—下、中二叠统;腕足Neospirifer ravana,Schizodus subquadratus,S.cf.elongatas,Parallelodon olseni,Pseudomonotis mongoliensis,Streblochondria?sp.,Palaeolima sp.,Myalinella cf.falcata等均见于内蒙古中部的早、中二叠世哲斯组。神螺滩双堡塘组的化石中没有发现典型的晚二叠世的特征分子。这一化石组合面貌显示神螺滩双堡塘组的时代应为早二叠世晚期—中二叠世,而不是晚二叠世。 相似文献
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本文简要总结了西藏措勤盆地相关区域的地层学研究进展。近年来,笔者及研究团队对措勤盆地及邻区进行了多次野外地质调查和室内古生物鉴定和研究,获得了一些新的发现和认识,在结合前人在相关地区取得的地层学成果和资料的基础上,厘定了该地区上二叠统—侏罗系的地层序列。措勤盆地的上二叠统是以文布当桑组为代表的灰岩和以木纠错组为代表的白云岩。三叠系存在着广海陆棚相和碳酸盐岩台地两种地层序列:前者自下而上划分为下三叠统嘎仁错组、中三叠统至上三叠统卡尼阶珠龙组、上三叠统诺利阶江让组、上三叠统瑞替阶至下侏罗统敌布错组;后者自下而上划分为木纠错组、待建的中三叠统、上三叠统诺利阶麦隆岗组和上三叠统瑞替阶至下侏罗统的确哈拉组。下侏罗统与上三叠统瑞替阶难以区分开。中侏罗统的岩性为深海-半深海相泥岩夹有基性-超基性岩。上侏罗统自下而上划分为萨波直不勒组和吐卡日组,目前尚未发现提唐阶的化石,因此推测下白垩统多尼组和吐卡日组之间有沉积间断。措勤盆地在晚二叠世—早三叠世、晚三叠世诺利期和晚侏罗世牛津期—基默里奇期都处于碳酸盐岩台地环境,冈底斯地区在中三叠世和中侏罗世发生了2期构造伸展事件,在晚三叠世诺利期末期和晚侏罗世基默里奇期晚期发生了两次构造抬升事件。构造伸展和挤压抬升造成了海平面的反复升降变化,导致了深水和浅水沉积相的垂向叠置,为油气成藏创造了良好的沉积建造组合条件。上二叠统—侏罗系地层序列还有待于进一步完善,应该加大地层古生物学的投入力度。 相似文献
11.
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