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1.
通过对柴达木地块天峻县组合玛地区晚二叠世13个采点的系统古地磁测定,揭示了一组高温特征剩磁分量.实验结果表明,采样剖面获得的晚二叠世古地磁结果具有正、反极性,其特征剩磁方向为:Dg=333.7°,Ig=37.3°,Kg=35.4,N=9,α95 =8.8;Ds=333.9°,Is=41.7°,Ks=69.9,α95 =6.2°,相对应的古地磁极位置为:64.0°N,342.4°E,A95=5.9°,古纬度为24.0°N.这一高温分量通过了倒转检验,我们认为这一高温特征剩磁分量很可能代表了研究区晚二叠世时期的原生特征剩磁.通过对比塔里木地块晚石炭-晚二叠世古地磁结果,发现两块体在晚石炭世存在明显的古纬度差(16.6±9.3°),而在晚二叠世其古纬度差(3.5±5.4°)在古地磁误差范围内并没有明显差别,从构造意义上说,说明柴达木地块在晚二叠世已是塔里木地块的一部分,结合地质资料,认为柴达木地块在晚二叠世时古地理位置处于塔里木地块的南缘或西南缘,这表明柴达木/塔里木地块间的古阿尔金断裂的形成时代不可能早于晚石炭世时,很可能形成于晚二叠世以后. 相似文献
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青藏高原羌塘地块和拉萨地块汇聚-碰撞拼合过程的研究对认识青藏高原中部隆升历史及其动力学过程具有重要的科学意义,而羌塘地块古地磁研究对理解上述问题至关重要。通过对羌塘地块西部改则地区晚三叠世灰岩的系统古地磁测定,获得其高温剩磁分量。但是这一高温剩磁分量未通过褶皱检验,表明为后期重磁化的结果。研究剖面高温特征剩磁平均方向在地理坐标下为Dg=349.3°,Ig=40.4°,κg=45.4,α95=6.5°,相应的古地磁极为76.4°N,311.1°E,dp/dm=4.7°/7.9°。这一古地磁极与羌塘地块早白垩世约110～100 Ma的古地磁极在古地磁误差范围内重合,表明其重磁化的时代为早白垩世约110～100 Ma。综合分析羌塘地块和拉萨地块古地磁结果,并结合海相地层、蛇绿岩和洋岛等地质证据,显示班公湖-怒江特提斯洋西段闭合的时间发生在早白垩世晚期约110～100Ma。改则地区晚三叠世灰岩的早白垩世晚期重磁化作用与羌塘/拉萨地块西部的碰撞密切相关。 相似文献
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通过对塔里木盆地内古董山地区早二叠世玄武岩的古地磁测定,揭示了1组高温特征剩磁分量。实验结果表明,其特征剩磁方向为：Dg=213.7°, Ig=26.9°,κg=19.7, N=9,α95=13.7°; Ds=217.7°, Is=-37.5°, κs=15.4,α95=13.6°,相对应的古地磁极位置为：53.2°N、 187.5°E,A95=12.3°,古纬度为21.0°N。由于采样剖面所获得的早二叠世古地磁结果全部为反极性特征,认为这一高温特征剩磁分量很可能代表了研究区早二叠世时期的原生特征剩磁。对比塔里木地块西北缘早二叠世的古地磁结果,认为研究地区与塔里木地块西北缘之间在古地磁误差范围内并未发生明显的相对构造运动。依据塔里木早二叠世古地磁极与哈萨克斯坦地块同时期古地磁极的一致性,结合二者的古生物资料,提出早二叠世时期塔里木地块可能已经与哈萨克斯坦地块碰撞相连,至晚二叠世,二者之间的海水完全退出,碰撞造山使得天山雏形基本形成。结合前人古地磁研究成果,对塔里木地块及周边主要块体早二叠世的古地理进行了重建。 相似文献
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内蒙古中部晚石炭世—早二叠世古地磁新数据及其地质意义 总被引：1，自引：0，他引：1
对采自内蒙古苏尼特左旗白音乌拉乡晚石炭世—早二叠世宝力高庙组和敖汉旗安庆沟乡晚石炭世酒局子组的凝灰岩和凝灰质砂岩开展了古地磁学研究。宝力高庙组和酒局子组样品退磁特征表明,高温剩磁分量均以赤铁矿为主要载磁矿物,可能携带了岩石形成时期的特征剩磁分量。层面校正后2个组平均特征剩磁分量分别为:D=159.3°,I=-33.1°,α95=8.7°;D=328.8°,I=31.3°,α95=5.7°。这反映了内蒙古中部晚石炭世—早二叠世位于北纬17°—18°N。将所获得的古地磁结果与已发表的相邻地区古地磁数据进行比较,并结合古生物、古气候等地质数据,推测晚石炭世—早二叠世时内蒙古中部与华北地块关系密切,距离较近,而远离西伯利亚地块,内蒙古中部晚石炭世—早二叠世时可能是华北地块的组成部分。 相似文献
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拉萨地块北缘尼玛地区晚白垩世古地磁结果及其构造意义 总被引：1，自引：1，他引：0
通过对青藏高原拉萨地块北缘尼玛县城附近晚白垩世红层8个采点的系统古地磁测定,获得了研究区晚白垩世可靠的古地磁数据。通过系统热退磁获得了采样剖面高温特征剩磁方向平均值为:Dg=9.9°,Ig=5.5°,κg=30.3,α95=10.2°,N=8(地理坐标下);D_s=8.2°,I_s=27.4°,κs=37.6,α_(95)=9.2°,N=8(层面坐标下);对应古地磁极为:71.2°N,241.9°E,dp/dm=5.5°/10.0°。该高温剩磁分量在地理坐标下与现代地磁场方向有显著差别,具有正、反极性,并通过了倒转检验,由此认为其很可能代表岩石形成时的原生剩磁。本次研究结果表明拉萨地块北缘在晚白垩世位于~14.5°N的古纬度位置(参考点:31.8°N,87.2°E)。对比稳定亚洲大陆参考极显示晚白垩世以来拉萨地块北缘与稳定亚洲大陆之间发生了1200±630km(10.9°±5.7°)的南北向构造缩短,但并未发生明显的相对旋转作用(0.8°±5.9°)。综合地质证据提出印度与亚洲大陆碰撞所造成的亚洲大陆内部南北向构造缩短主要集中在拉萨地块以北的区域。 相似文献
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塔里木地块上石炭统的古地磁研究 总被引：3，自引：1，他引：2
本文对塔里木地块西北缘柯坪地区的3条上石炭统康克林组剖面进行了古地磁研究。95个定向岩心样品的逐步热退磁和交变退磁揭示出3个磁性组分,第一个是具有低解阻温度谱或低矫顽力谱在现代地磁场作用下形成的粘滞剩磁A(D=10°;I=56°,α95=4°);第二个是红色石英砂岩的具有反极性的高温组分B(D=217°,I=-43°,λ=56°,Φ=184°E;A25=6°详细研究表明,该分量受附近晚二叠世脉岩侵入的重磁化;第三个是灰岩高矫顽力谱的反极性组分C（D=241°、I=-51°,λ=41°N,Φ=160°E,A（?）=4°）。这一分量通讨倾斜检验,在95%概率水平上明显不同于塔里木地块目前已有的石炭纪以后的古地磁方向,它代表了原生剩磁。研究结果表明:（1）晚石炭世塔里木地块已和哈萨克斯坦地块、苏联西天山地块以及西伯利亚地块发生碰撞:（2）苏联西天山地块相对塔里木地块曾逆时针旋转了70°（欧拉极位置λ=8°N,Φ=69°E）,而塔里木地块则相对西伯利亚地块逆时计旋转了21°（欧拉极位置λ=20°N,Φ=34°E）。从该区已有的晚古生代至早三叠世占地磁数据看,这些地块之间的相对旋转运动发生于早三叠世之后。 相似文献
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青藏高原拉萨地块早白垩纪火山岩古地磁结果及其构造意义 总被引：1，自引：1，他引：0
对青藏高原拉萨地块早白垩纪火山岩15个采点的古地磁测定,揭示了一组高温特征剩磁分量.实验结果表明采样剖面获得的早白垩统卧荣沟组的古地磁结果全部为正极性,显示与早白垩纪正极性超静带的极性特征相似.对岩石的显微镜观察表明岩石未受后期热液化学交代作用和风化作用,这表明所获得的高温分量很可能代表岩石形成时的原生剩磁.其特征剩磁方向为:偏角D=18.4°,倾角I=26.5°,α95=8.6°;相应的极位置为:经度ψp=220.3°E,纬度λp=66.4°N,dp=9.3°,dm=6.9°,古纬度plat=14.0°.通过对比拉萨地块以北诸地块早白垩纪古地磁结果,认为拉萨地块在早白垩纪已与芜塘地块碰撞拼合在一起,而自早白垩纪以来相对欧亚大陆发生了1500±600km的构造缩短.结合拉萨地块已有的晚白垩纪和古新纪古地磁数据,认为欧亚大陆的最南缘(拉萨地块)在印度/欧亚大陆发生碰撞前自早白垩纪一始新纪一直处于北纬12.8°～14°N低纬度位置,并未发生明显的纬向运动. 相似文献
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报道拉萨地块西段三叠纪古地磁研究的初步结果。古地磁样品来自措勤县敌布错北缘新发现的海相三叠纪地层,共采集6个采点67块独立定向样品。岩石磁学实验表明,样品中含有大量中低矫顽力中等阻挡温度的磁性矿物和一定量的磁铁矿。于4个采点的47块样品中分离出现代地磁场的低温粘滞剩磁(分量A),在6个采点66块样品中获得白垩纪的次生剩磁分量(分量B),5个采点28块样品获得高温特征剩磁分量(分量C)。分量C仅可在少数以磁铁矿为主要载磁矿物的样品高温区间(525~585℃)获得,可通过标准褶皱检验,为岩石形成时期的原生剩磁信息。计算得出拉萨地块三叠纪的古地磁极位置:φρ=17.4°N、λρ=205.9°E、(dp=6.7,dm=3.7),该结果表明拉萨地块三叠纪处于南纬中低纬度地区。结合羌塘古地磁结果推测,羌北地块与拉萨地块之间班公湖—怒江缝合带所代表的特提斯洋盆可能在早三叠世打开,早三叠世—晚三叠世期间快速扩张并推动羌北地块快速北移,促使了羌北地块与欧亚大陆南缘的拼合。 相似文献
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选择龙门山构造带剑阁县竹园镇马鹿乡地区早三叠世飞仙关组,开展了详细的古地磁研究。通过对飞仙关组9个采样点灰岩、泥质灰岩样品系统的古地磁测试,热退磁结果分离了一组高温特征剩磁分量。样品的高温剩磁分量具有正、反双极性,且通过了倒转检验,表明它们很可能代表了岩石形成时的原生剩磁。构造校正后的特征剩磁方向为:偏角D_s=42.3°,倾角I_s=12.6°,α_(95)=9.4°;相应的极位置为:经度φ_p=219.3°E,纬度λ_p=42.9°N,d_p/d_m=4.9°/9.6°,古纬度plat=6.4°。对比稳定的四川盆地早三叠世的古地磁结果,获得龙门山构造带相对于稳定四川盆地发生了1.2°±4.4°的顺时针旋转运动,为此从构造古地磁角度,提出龙门山构造带和四川盆地自早三叠世以来,在动力学上已是统一的构造单元,并没有发生明显的构造旋转作用。 相似文献
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海南岛白垩纪古地磁结果及其构造地质意义 总被引：5，自引：0，他引：5
对海南岛地区白垩系鹿母湾组和报万组碎屑岩219个独立定向岩芯样品(29个采点)的岩石磁学和古地磁学研究表明,白垩纪的碎屑岩以赤铁矿为主要载磁矿物。逐步热退磁分析表明,绝大多数样品可分离出特征剩磁分量。综合前人的结果,获早白垩世特征剩磁方向D=6.5°,I=42.7°,κ=73.4,α95=8.2°;晚白垩世特征剩磁方向D=6.7°,I=44.7°,κ=125.5,α95=5.4°。其早白垩世古纬度24.8°(+6.2°/-5.8°),晚白垩世古纬度26.3°(+4.6°/-4.0°);均位于现在地理位置以北约5°～6°。与华南板块东南缘白垩纪的古地磁数据对比表明,晚白垩世海南地块仍是华南板块的一部分。海南岛白沙断裂东西两侧早白垩世古地磁数据的差异,表明存在一个北东向的构造走滑带,白沙断裂可能是华南沿海北东向构造带的南延部分。海南岛白垩纪古地磁结果也表明,相对印支地块,海南岛在早白垩世时发生了25°左右局部顺时针旋转。推测此局部旋转很可能与晚侏罗世—晚白垩世早期,印度洋开始第一次海底扩张,印度板块向北运动有关。 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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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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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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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
17.
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
18.
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
19.
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