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1.
新城－黄陂走滑韧性剪切带的动力分异作用 总被引：2，自引：0，他引：2
谭秋明 《大地构造与成矿学》1995,19(2):171-177
本文通过对新城－黄陂断裂带中合河－殷店右行走滑韧性剪切带内糜棱岩类岩石化学成分、稀土元素及微量元素随Ｓｓ－Ｓｃ夹角和古差异应力（△δ）的变化梯度的研究，初步探讨了右行走滑韧性剪切带的动力分异作用。 相似文献
2.
桐柏-大别南缘变质流体变质-变形特征及构造意义 总被引：1，自引：0，他引：1
前人研究认为桐柏山主要是由桐柏核部杂岩单元组成,它是一个早白垩世花岗质片麻岩杂岩体,其中包含一定的三叠纪中高级变质岩石,后期一起经历相同的构造变形过程,在南北两侧形成剪切旋向完全相反的两条大型韧性剪切带,殷店-马垅剪切带就是南边的华南板块由SSE→NNW挤压作用下,在斜切大别造山带的方向上产生的右行平移断裂带。在野外进行地质考察的过程中,发现在该地区变质流体的分布具有一定的规律。因此,本文通过对殷店-马垅剪切带地质特征、走滑性质、糜棱岩及糜棱岩化岩石的变质变形,剪切带内长英质脉体物质组成、变形特征及物质来源等方面研究,探讨剪切带中变质流体的分布规律以及变质变形与变质流体之间的关系。 相似文献
3.
广东河台金矿构造应力场演化及构造控矿模式 总被引：3，自引：1，他引：2
广东河台金矿位于两广云开大山地区吴川-四会断裂变质带与广宁-罗定断裂变质带交汇部位,为一典型的韧性剪切带蚀变糜棱岩型金矿。海西-印支期区域SN向左旋挤压应力形成有区域左行韧性剪切性质的吴川-四会断裂变质带和广宁-罗定断裂变质带;燕山早期,区域构造应力转为SN向右旋挤压,区域韧性剪切带转为右行韧性剪切性质,并对先期形成的糜棱岩带改造显示为右行剪切特征;燕山晚期,大规模的右行韧性剪切活动逐渐转为右行脆-韧性、脆性剪切,在部分糜棱岩带中产生脆性断裂。河台金矿严格受韧性剪切糜棱岩带控制。区域吴川-四会断裂变质带和广宁-罗定断裂变质带是一级构造,两者交汇部位控制了河台金矿田的产出;燕山期,广宁-罗定断裂变质带的C-R次级构造（即河台韧性剪切带及其糜棱岩带）是二级构造,控制了河台金矿床的分布;河台矿区糜棱岩带中的张剪裂隙和主剪切裂隙系统是第三级构造裂隙,控制了河台金矿床的类型(蚀变糜棱岩型和石英脉型)及金矿体的分布和形态。 相似文献
4.
殷马断裂带在桐柏山—大别山造山带中的地质意义探讨 总被引：2，自引：0，他引：2
殷店—马垅断裂带是桐柏—大别造山带南缘一条重要的韧性断裂带,是桐柏—大别造山带内部发育的一条明显的岩地层单元界线,同时也是华北和扬子两大板碰撞挤压的产物。它与桐柏—大别造山带的形成,发展和演化,有着密不可分的联系。通过对殷店—马垅断裂带东西段野外岩性剖面对比分析、显微构造对比、有限应变测量对比分析、应力场分析等,发现尽管东、西段构造特征略有差异,但是殷店—马垅断裂整体是具有右旋运动性质的剪切带,殷店—马垅断裂带的形成对华北与扬子碰撞所产生的应力具有消减转移效应,它本身是一个塑性剪切最强的断裂带,它反映了造山带内部不同岩性的块体之间右旋流变的运动学模式,同时也可能充当着桐柏—大别山核部岩块相对扬子板块向东运动的的"润滑带"。 相似文献
5.
桐柏杂岩的南北边界的剪切带分别是殷店-马垅韧性剪切带和晓天-磨子潭韧性剪切带,这两条韧性剪切带内都发育杆状构造,且杆状构造具有层状结构,层与层之间通过一种特殊的滑脱面结合。由于晓天-磨子潭韧性剪切带相对于殷店-马垅剪切带位置明显更靠近商丹断裂带,早期商丹断裂带的活动在岩石中留下的变形痕迹导致了后期晓天-磨子潭韧性剪切带的变形程度要略强于殷店-马垅剪切带。这两条剪切带都是以简单剪切为主的剪切带,变质条件也相似,都属于角闪岩相变质,处于中-下地壳流变层位置。U-Pb同位素测年结果显示,晓天-磨子潭韧性剪切带的活动年龄为171~142Ma,殷店-马垅韧性剪切带的活动年龄为164~137Ma,两条剪切带的主活动期都在中-晚侏罗世,在早白垩世随着岩浆活动的峰期到来慢慢减弱停止。桐柏造山带在印支晚期碰撞挤压背景下的向东挤出不是一个整体的挤出,而是有层次的差异挤出,挤出的同时层与层之间会发生滑动,滑脱面类似滑动的润滑剂,酷似"管状流动"的构造。在晓天-磨子潭韧性剪切带和殷店-马垅韧性剪切带的牵引作用下,整个桐柏造山带由西向东发生管状流动。 相似文献
6.
吴川－四会断裂是我国华南一条重要的深大断裂兼控矿构造，沿带分布了一系列大型、超大型金属矿床，同时与粤北铀矿成矿有着十分密切的关系。本文在论述了它作为一条大型对冲韧性剪切带的一系列特征后指出，它与其他构造的交汇复合是控制矿产分布的重要构造条件，并提出了韧性剪切带、拉伸构造、铀活化区、幔涌带＂四位一体＂的铀成矿构造模式。 相似文献
7.
辉发河—古洞河断裂是吉林省境内华北地块的一条界限断裂。野外地质、显微构造及同位素资料表明,沿该断裂两侧出露的台槽两区的岩石经历了由早期的韧性变形到晚期脆性碎裂这样一个长期复杂的变形变质过程,它们是不同深度层次的断裂构造特征在地表的反映。吉林省金矿集中分布于该剪切带中,二者构成一个应变统一体。所以,糜棱岩、确定断裂构造环境是远景找矿的重要条件。前人为此做了大量卓有成效的地质找矿工作。本文根据1982～1984年对吉林省金矿成因研究的实际资料,在综合区域构造、矿区构造和显微构造分析的基础上,提出了辉发河—古洞河断裂性质为韧性剪切带,金矿为韧性剪切带金矿的粗浅看法。 相似文献
8.
殷店-马垅（简称殷马）韧性剪切带是桐柏-大别造山带南缘的一条重要的边界断裂,对其精细的构造变形研究将有助于进一步认识桐柏-大别造山带的演化方式和过程。本文主要对殷店和马垅两个地区进行了详细的剖面观测,利用有限应变测量,计算出殷马剪切带中岩石应变椭球长短轴的平均轴率为1.69,靠近剪切带的岩石应变量大,向北远离剪切带,应变量减小;通过构造应力场分析查明剪切带的古应力状态,最大压应力σ1为北北东-南南西向,对应最大拉应力σ3为北西西-南东东向。岩石的有限应变分析和应力场状态,反映出板块间的碰撞挤压作用力在平行剪切带和垂直剪切带方向上存在应力分解。剪切带内糜棱岩中的锆石U-Pb定年结果显示,其年龄为172～137 Ma,据此得出殷马剪切活动时代主要为中侏罗世-早白垩世。 相似文献
9.
小北湖韧性剪切带分布于敦密断裂北侧泥盆纪地层中,为逆冲推覆韧性剪切带,发育各种糜棱岩、叶理和线理构造及显微构造,其变形机制为简单剪切变形,属低温韧－－脆型剪切带。 相似文献
10.
吴川—四会断裂北段特征及其与金属成矿的关系 总被引：1，自引：0，他引：1
吴川－四会断裂是我国华南一条重要的深大断裂兼控矿构造，沿带分布了一系列大型，超大型金属矿床，同时与粤北铀矿成矿有着十分密切的关系，本在论述了它作为一条大型对冲韧性剪切带的一系列特征后指出，它与其他构造的交汇复合是控制矿产分布的重要构造条件，并提出了韧性剪切带，拉伸构造，铀活化区，幔涌带“四位一体”的铀成矿构造模式。 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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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
14.
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
15.
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
16.
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
17.
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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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
20.
Michel Westphal Mikhail L. Bazhenov Jean Paul Lauer Diamar M. Pechersky Jean-Claude Sibuet 《Tectonophysics》1986,123(1-4)
We first re-examined the apparent polar wander curves for stable Eurasia and Africa since the Triassic. These curves were then combined together with curves of North and South America according to the kinematics of the Atlantic ocean and a synthetic polar wander curve was given. Then, most of the paleomagnetic results from the Tethys mobile belt, from the Atlantic to the Pamirs, were analysed.Several groups of plates, microplates and blocks can be seen. First, relatively stable regions like Maghreb and Sicily, which have not moved much. Then we have a group formed by Iberia, Sardinia, Italy and, to a lesser extent, Corsica and the Western and Central Alps. For these blocks, movements are anticlockwise rotations chiefly driven by the anticlockwise rotation of Africa, but they are sometimes stronger.To the east, a major change takes place. The north of the Aegean Sea and the Ionian zone are clockwise rotated and these rotations are recent: Oligocene-Miocene for the first part, Pliocene to the present for the second part.A major problem arises in Turkey, Caucasus and Iran. Paleomagnetic results indicate a position far to the south of Eurasia, and, at the same time, geological evidence is in favour of a position close to Eurasia. We discuss these discrepancies. 相似文献