大断面深埋高水压地铁盾构隧道周边土压力作用模式评价

以南京某大直径地铁盾构隧道为背景,对盾构管片衬砌所受荷载及结构内力进行现场测试,分析了深埋高水压粉细砂地层中盾构隧道管片土压力大小及分布特征。采用3种不同竖向荷载组合（即有效上覆土压力+水压力,太沙基松动土压力+水压力,只有水压力）计算管片内力并与实测内力进行比较,评价了作用在盾构隧道管片上的土压力模式。结果表明：（1）作用在盾构隧道衬砌上的水压力大小基本等于静止水压力;（2）盾构隧道隧顶实测土压力约为太沙基松动土压力的80%,实测隧顶土压力更接近于太沙基松动土压力,隧道上方存在土拱;（3）现场实测管片弯矩较3种荷载作用下计算弯矩小,而实测管片轴力约为理论计算轴力的2倍。此外,分析了水平地基抗力系数对隧道管片内力的影响。研究成果可为大直径深埋盾构隧道设计提供参考。     

盾构隧道实测土压力分布规律及影响因素研究

以大量现场实测土压力为基础,分析了影响盾构隧道衬砌土压力的一些主要因素,总结出不同地层地铁盾构隧道长期稳定土压力的分布规律,并探讨了盾构施工期土压力随时空的变化情况。研究得出,地下水位高低对稳定土压力大小及分布影响较大;作用在管片上的长期土压力大小与地层衬砌刚度系数有关,当地层衬砌刚度系数为1.5时,管片竖向及水平土压力都较小;盾构施工期临时荷载对管片土压力影响不可忽视,无论是黏土地层还是砂土地层,大的注浆压力及注浆率将导致作用在管片上的稳定土压力分布不均;管片土压力可按时空分为4个阶段,拼装阶段、同步注浆阶段、浆液凝固阶段及后期稳定阶段,其中同步注浆阶段管片周边最大土压力为稳定阶段的2～3倍。     

复合式衬砌结构中衬砌分担围岩压力比例的研究

复合式衬砌结构中衬砌分担围岩压力的评价方法是隧道工程技术的重要研究课题之一。依托某新建铁路隧道工程,提出了一种基于监测位移反分析评价围岩和支护应力,进而计算初期支护和衬砌背后压力的方法。根据监测位移和衬砌施作时间,确定初期支护的已发生变形和剩余变形。通过有限元反分析求出与已发生变形和剩余变形相对应的围岩和支护应力,得到初期支护和衬砌背后压力。对比初期支护背后压力及衬砌背后压力的现场监测和反分析的计算结果,两者比较一致,说明了该方法的可行性。该新建隧道初期支护闭合95 d后施作衬砌,计算得到衬砌背后压力约0.04～0.06 MPa,衬砌分担围岩压力比例约13%～16%。研究成果对复合式衬砌结构的设计具有一定的参考意义。     

黄土地层盾构隧道受力监测与荷载作用模式的反演分析

为探明黄土地层中地铁盾构隧道管片衬砌结构与周围土体的相互作用关系,以西安地铁2号线穿越老黄土地层盾构隧道为研究对象,对实际作用于管片衬砌结构的水压力、土压力及主体结构内力（轴力、弯矩）进行现场动态跟踪测试,分析施工过程中盾构机动态掘进及后期稳定后的土-水压力对管片结构受力的影响。结合利用管片内力的现场实测值,采用正交试验设计分析方法,定义优化分析函数,反演分析黄土地层中盾构隧道管片衬砌结构设计荷载的合理计算参数。通过对比分析表明,运用优化后的设计参数得出的计算内力值与实测值在量值与分布上均较为接近,证实了分析方法的可行性、合理性,其成果可供类似工程设计参考。     

水工隧洞钢筋混凝土衬砌外水压力取值方法研究

外水压力是隧洞衬砌承受的主要荷载之一,也是控制其建设与运行或检修过程中衬砌结构安全的关键因素。目前外水压力的取值仍然以经验公式为主,存在很大的局限性和不准确性。首先分析对比了衬砌外水压力的折减系数法、理论解析方法和数值分析方法几种取值方法,然后进行了不同渗透环境和衬砌支护条件下的衬砌外水压力计算。结果表明,随着围岩渗透性和衬砌厚度的增大,衬砌外表面的水压力越大;对于渗流数值计算,模型范围应取距离隧洞中心不小于30倍洞径;考虑渗流场的时间效应,开挖完成10 d后隧洞的渗流场趋于稳定,衬砌支护20 d后衬砌外侧水压力分布趋于稳定。     

西安地铁正交地裂缝隧道的模型试验研究

以西安地铁二号线穿越地裂缝的区间隧道为对象,通过几何相似比尺50:1的物理模型试验,开展了地裂缝活动条件下地铁隧道骑缝（变形缝与地裂缝一致）正交穿越地裂缝时衬砌结构与围岩相互作用机制的试验研究。结果表明,在地裂缝发生各级错动位移条件下,不同围岩应力场的围岩土压力、衬砌结构应力及其不均匀沉降位移变化规律相似;上下盘内的衬砌结构之间具有明显的错断位移,下盘内衬砌结构的沉降量越小,上盘内衬砌结构的沉降量越大,均呈渐变趋势;上盘内衬砌结构应力、围岩土压力随地裂缝错动位移的增加而减小,下盘衬砌结构应力和围岩土压力随地裂缝错动位移的增加而增大,围岩土压力和衬砌结构应力的增量峰值均发生在地裂缝附近。模型试验研究研究结果对于分析地裂缝活动区间地铁隧道工程的运营及维护具有重要的理论与实际意义。     

盾构隧道管片衬砌荷载模式比较分析

地下结构的荷载分布计算是非常复杂的 ,针对上海某越江盾构隧道 ,采用梁—弹性铰—地基系统计算模型 ,就水土压力合算与分算、侧向土压力和水压力的分布形式等设计了几种荷载模式 ,并分别计算分析比较了管片衬砌结构在这些荷载模式作用下的内力分布和变形特性 ,并从中得出了一些有价值的结论。     

成层土中悬臂式地下墙内力计算等等值梁法

建筑基坑范围内的土层以成层土居多，基坑技术规范要求计算成层土的土压力时应分层计算，本文按等值梁法原理，给出了成层土中分层计算土压力，再计算悬臂式地下连续墙支护结构内力（剪力和弯矩）的方法。     

爆炸荷载作用下深埋圆形隧洞的饱和黏弹性土-衬砌系统动力响应

假定土骨架服从标准线性固体黏弹性本构关系,研究了深埋圆形隧洞的饱和黏弹性土-弹性衬砌耦合系统在轴对称爆炸作用下的瞬态动力响应。首先,基于饱和土的Biot模型和衬砌的弹性理论,通过引入势函数和Laplace变换,利用弹性衬砌和饱和黏弹性土界面处的连续性条件以及边界条件,得到饱和黏弹性土体和弹性衬砌位移、应力和孔隙水压力等在Laplace变换域中的解析解。其次,利用Laplace数值Crump逆变换得到耦合系统在时间域的动力响应,数值分析了不同土体模型下土体-衬砌耦合系统的径向位移和环向应力以及土体孔隙水压力等。结果表明：对不同土体模型的土体-衬砌耦合系统,其在爆炸载荷作用下的动力响应性态基本一致,但动力响应的振动周期和幅值等具有明显的差异。同时,对于饱和黏弹性土-弹性衬砌系统,土体黏性参数对土体径向位移和孔隙水压力有明显的影响,但对土体环向应力影响较小。     

涵洞顶填土压力的计算分析

简要介绍了圆管涵破裂的原因，论述了根据公路规范、铁路规范计算涵洞顶场土压力的方法及其缺陷，提出了种新的涵洞顶场土压力计算方法。计算结果表明，该方法克服了上述两种规范中计算方法的不足。     

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.     

Global repeating events in the history of the Earth and the motion of the Sun in the Galaxy

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.     

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″.     

从榴辉岩与围岩的关系论苏鲁榴辉岩的形成与折返

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。     

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。      

摩擦桩基桩土间极限摩阻力取值问题探讨

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。     

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.     

On the consistency of proposed models for the Pyrenees with the structure of the eastern parts of the belt

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.