基于遗传算法的抗滑桩优化设计

抗滑桩由于其桩位布置灵活、施工比较方便、治理效果可靠,是滑坡治理工程中广泛采用的一种抗滑措施。一直以来抗滑桩设计都是沿用手工查表计算的方法,采用这种传统的抗滑桩设计方法不仅增加了工程师繁重的计算工作,而且很难实现优化设计。文章在对抗滑桩的工作机理进行分析的基础上,讨论了影响抗滑桩经济性的主要因素,以抗滑桩的截面宽、高和长度为基本要素,建立了抗滑桩优化设计的数学模型,并采用遗传算法进行求解。最后对一个工程实例用传统设计方法和优化设计方法所得的结果进行了比较,结果表明,对抗滑桩进行优化设计不仅能减轻工程设计人员的工作量,还可以在满足安全的条件下明显的降低工程费用,在滑坡治理工程中具有一定的实际意义。     

面向对象有限元程序设计及其VC++与Matlab混合编程实现

应用面向对象方法来研究有限元,是对有限元新方法的有益尝试和创新性发展。通过对比面向过程和面向对象的程序设计方法,讨论了面向对象方法与有限元程序设计相结合的优点,并简要回顾了国内外面向对象的程序设计方法的研究进展。应用面向对象的程序分析方法,建立了三维脆塑性有限元分析类库。采用VC 和Matlab混合编程的手段,设计了基于Windows98/2000/NT操作平台的面向对象的三维脆塑性有限元分析软件,成功地分析了国内某大型水电站地下硐室群围岩稳定性,验证了该面向对象有限元分析程序的有效性和实用性。     

油藏多相渗流的面向对象有限元程序设计

近年来,面向对象的编程技术越来越受到人们的重视,并用来解决和模拟各种物理问题和工程问题,特别是在有限元方法编程和模拟中得到了广泛地应用。介绍了面向对象的程序设计方法和它与有限元程序相结合的原理和优点。在此基础上提出了面向对象有限元方法在油藏多相渗流中的应用实例,并按照面向对象的程序设计方法,基于Windows XP平台采用Visual C++.NET语言,建立了有关描述多相渗流的有限元模型的类,给出了类的描述和它的实现方法。建立的相关类及其实现方法主要包括处理矩阵计算的类、节点类、单元类、材料类、形函数类等。据此编制了油藏多相渗流的有限元分析的数值计算程序,并给出了一个数值实例。     

面向对象有限元方法在岩土工程中的应用

介绍了面向对象的程序设计方法和它与有限元程序相结合的原理和优点,提出了这种方法在岩土工程中的应用实例,并设计了基于Windows 95/98平台的有限无软件。利用面向对象的方法来研究有限元,是对有限元方法新的有益尝试。     

基于有限差分法的抗滑桩计算机辅助设计

基于地基系数“m-m”法、“m-k”法、“k-k”法的原理,考虑桩顶和桩底边界条件以及桩在滑动面处位移、转角、弯矩和剪力的连续条件,可解得桩身各节点的位移和内力,提出了进行抗滑桩全桩内力计算的有限差分法。根据差分方程并用VB6.0编制了实用的计算程序,既可避免繁琐的查表计算,提高计算速度,又可提高计算精度,直观生动,真正实现了人机交互,在界面的引导下,设计人员可完成全部计算,并绘出内力图形和抗滑桩截面配筋图,使设计更方便快捷,该软件可以极大地提高生产效率,降低工程造价,从而实现抗滑桩的优化设计。最后采用上述方法对某滑坡的悬臂抗滑桩进行了设计与计算。     

滑坡稳定性评价及治理工程设计软件Slope Designer

主要介绍了Slope Designer 1.2的设计开发思路和主要功能.该软件是基于Windows面向对象技术开发的滑坡稳定性评价与治理工程设计的一体化工程软件,采用Visual C 进行程序设计,包括稳定性分析子模块和抗滑桩设计子模块2部分,可对地震作用、暴雨等不同工况下的滑坡进行稳定性评价和推力计算,并能够对(锚拉)抗滑桩(弹性桩、刚性桩)的弯矩、剪力及侧应力进行计算,最后根据内力计算结果完成配筋计算.在三峡库区兴山县二里半滑坡的应用研究表明,该软件具有很好的工程实用性.     

考虑滑床复合倾斜岩体综合地基系数的抗滑桩受力特征研究

在抗滑桩内力与变形计算中,当前理论分析多将滑床岩体等效成均质体或水平的非均质体,而三峡库区大部分滑床多为复合倾斜岩体。通过3DEC数值试验,研究了抗滑桩的有效影响范围与桩截面宽度、深度的关系,确定了抗滑桩有效影响范围的上、下限;利用面积等效,在桩的有效影响范围内提出了滑床复合倾斜岩体综合地基系数K_(Zi)的公式;推导了基于K_(Zi)的弹性抗滑桩嵌固段受力特征研究的计算公式并编写了MATLAB计算程序。以马家沟滑坡为例,采用等效法、水平层状地基系数法和基于K_(Zi)的计算方法分别进行了抗滑桩嵌固段内力、位移的计算。结果表明,基于K_(Zi)的计算方法与水平层状地基系数法相比,滑面处位移增大14.6%,内力相差较小;同时,基于K_(Zi)的计算方法根据滑动面处的位移反求桩顶的位移与现场监测位移较为接近,而利用传统方法计算位移偏小,设计偏于危险。该方法可为复合倾斜岩体地区的抗滑桩设计提供理论支撑。     

考虑预应力损失桩-锚结构内力计算的加权残值法

针对已有锚索抗滑桩计算模型的不足,按锚索抗滑桩实际的受力过程,考虑了施工阶段锚索预应力的损失及桩体位移对桩锚协调方程的影响,分别在预应力施加和滑坡推力作用阶段建立计算模型,并基于加权残值法建立了锚索抗滑桩的内力与变形计算方法。同时,基于Matlab平台编制了锚索抗滑桩的计算程序,将该程序对已有的工程实例进行分析,并与现有的桩锚计算模型进行对比,结果表明,该模型能很好地体现锚索抗滑桩在预应力施加阶段主动受力这一特殊过程对桩锚位移协调方程的影响,且能考虑下排锚索施工对上排锚索造成的预应力损失;而且与现有的计算模型相比,本模型更加符合工程实际。     

基于可靠性理论抗滑桩设计体系的研究

抗滑桩设计的常规方法是建立在定值基础上的,未能考虑计算参数的随机性与变异性,故在抗滑桩设计中存在局限性：一是不能给出抗滑桩设计的边坡安全度;二是设计中过分保守,造成浪费。可靠性分析法考虑了计算参数的随机性,用严格的概率来度量边坡的安全度,弥补了上述传统抗滑桩设计中存在的不足。基于可靠性分析法,以传统边坡稳定性计算公式为基础,建立了抗滑桩设计的边坡稳定性评价模型,并且运用蒙特卡罗法,采用单参数敏感性分析方法,分析抗滑桩设计各参数对边坡安全系数及可靠性指标的影响。结果表明,岩土体抗剪强度参数、岩土体重度、抗滑桩直径等因素对可靠性指标影响较明显,边坡安全系数对岩土体重度、抗滑桩有效长度、抗滑桩直径等随机变量较敏感。     

考虑滑床不同地基系数的抗滑桩受力特征研究

基于目前在抗滑桩理论研究方面多将滑床层状地层等效成均质体,在多层地基横向受荷桩挠曲微分方程的基础上,推导出考虑滑床不同地基系数的弹性抗滑桩嵌固段变位、内力和应力计算的公式。用Matlab软件编写了抗滑桩变位、内力和应力计算与图形处理程序,有效提高了抗滑桩变位、内力和应力分析效率和计算精度。工程实例表明,考虑滑床不同地基系数计算方法对比等效法,滑面处位移、滑面处转角、剪力最大值、弯矩最大值分别增大25.76%、18.04%、14.90%和4.16%,而滑动面处桩侧应力较等效法减小44.91%。该研究成果对滑坡为不同岩性的岩体进行抗滑桩设计具有指导意义。     

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.     

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″.     

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.     

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。     

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。      

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.