青藏铁路多年冻土工程地质综合分类探讨

根据影响青藏高原多年冻土工程特性的地温分区和冻土类型，提出了冻土工程地质综合分类方法，结合青藏铁路多年冻土区工程设计和施工情况的实践，对铁路建设中如何应对全球气温变暖下冻土区工程安全提出了工程措施。     

影响青藏铁路冻土区主要工程措施可靠性的气温变化指标分析

多年冻土是气候条件控制的特殊地质体,气温升高和降水条件变化将对青藏铁路沿线的多年冻土产生深刻影响.从全球气温变化背景和青藏高原气候变化的实际情况出发,分析和论述了气候变化对青藏铁路沿线多年冻土地温特征及冻土区工程建筑物的可靠性产生缓慢而持续影响的气温变化指标.通过对冻土区工程设计原则和工程结构、工程措施可靠性产生重大影响的气温变化特征的分析,提出对目前冻土工程可靠性的看法,并提出应对工程措施.     

青藏铁路多年冻土工程的研究与实践

青藏铁路建设需穿越高原多年冻土区, 在探明沿线多年冻土分布特征的基础上, 合理确定了青藏铁路线路的走向方案.在多年的冻土研究和工程实践的指导下, 有针对性地开展了 5 个不同类型冻土工程试验研究, 取得重要科研成果, 指导设计和施工.全面总结4 a来青藏铁路多年冻土工程的研究与实践, 提出了“主动降温, 冷却地基, 保护冻土”的设计思想, 制定了路基、桥涵、隧道成套工程技术措施和先进施工工艺, 对确保多年冻土工程质量发挥了重要作用.     

青藏铁路普通路基下部冻土变化分析

高温高含冰量冻土地区,青藏铁路采取了冷却路基、降低多年冻土温度的工程措施.然而青藏铁路仍有大量路段未采用任何工程措施,因此修筑普通路基后冻土变化也是普遍关心的问题.根据青藏铁路普通路基下部土体温度监测的近期结果,分析了季节冻土区、已退化多年冻土区和多年冻土区路基下部冻土变化特征.结果表明,不同区域修筑普通路基,其下部土体温度、最大季节冻结深度、多年冻土上限等存在较大的差异.在季节冻土和已退化多年冻土区,右路肩下部(阴坡)已形成冻土隔年层;在多年冻土强烈退化区,其路基下部形成融化夹层;在高温多年冻土区,其路基下部上限存在抬升和下降,上限附近土体温度有升高的趋势.在低温多年冻土区,其路基下部上限全部抬升,上限附近土体存在"冷量"积累,有利于路基下部多年冻土热稳定性.因此,低温多年冻土区修筑普通路基后,冻土变化基本是向着有利于路基稳定性的方向发展,在其它地段修筑普通路基,冻土变化是向着不利于路基稳定性的方向发展的.特别是阴阳坡太阳辐射差异,导致了土体热状态和多年冻土上限形态产生较大的差异,这种差异将会对路基稳定性产生一定的影响.     

青藏铁路多年冻土区工程复杂性分析

青藏铁路穿越550km多年冻土区,多年冻土地温、冻土类型以及沿线生态环境等存在较大的差异,使多年冻土区工程较为复杂。因此本文提出了冻土工程复杂性概念,建立冻土工程复杂性评价模型,并利用GIS平台对青藏铁路沿线唐古拉山越岭地段工程复杂性进行了分析和研究。研究结果表明,青藏铁路穿越的唐古拉山越岭地段工程复杂性相对较小,而青藏公路的工程复杂性相对较大。这表明了青藏公路沿线冻土工程比青藏铁路沿线更为复杂,在各种因素的影响下,青藏公路路基稳定性变化比青藏铁路更加复杂。     

煤矿开采过程中的冻土环境问题与对策

冻土区矿产资源的开发,对多年冻土的影响速度快、范围广、最直接,是其他人为活动无法比拟的.特别是煤矿开采,它对多年冻土影响剧烈,使得煤矿区冻土环境更加脆弱.青海木里煤田矿区处于青藏高原阿尔金山—祁连山高寒带山地多年冻土区,是大通河上游水源涵养生态功能区,冻土生态环境较为敏感.在分析青海木里煤田矿区多年冻土分布状况与特征的基础上,从多年冻土变化和多年冻土区自然环境变化两个方面,探讨了煤矿开采过程中的冻土环境问题,并提出避免和减缓煤矿开采对冻土环境造成影响的建议与对策,以期为寒区资源合理开发利用保护提供科学依据.     

青藏高原多年冻土区路基工程地质研究

回顾了青藏高原多年冻土区近年来所开展的路基工程地质研究工作,指出冻土工程地质勘探在方法上有很大进展,总结出了一整套冻土区工程地质勘察的暂行规定和细则.近年来的工作特别注重了对冻土地温和含冰量的研究,这是冻土工程地质中特有的十分重要的参数.在大量观测试验的基础上,总结出了有关路基稳定性的若干重要结论.据此提出,在气候转暖的背景下,高温冻土区筑路必须采用"冷却路基"的方法.为寻求气候转暖的对策,冻土工程地质预报的研究也取得了很大的进展,对冻土区路基工程地质的研究方向提出了新的建议.     

青藏铁路冻土区环境问题对工程安全可靠性影响

本文分析了青藏铁路冻土区主要工程对多年冻土温度、水分特征和冻土环境特征的影响,探讨了冻土区工程环境与冻土环境之间相互作用特点。进而论述了控制外界对冻土工程环境系统的热侵蚀是保证冻土区工程安全可靠性的关键问题。     

多年冻土地区机场跑道修筑技术现状

我国分布有大面积的多年冻土, 根据我国机场建设的中长期规划, 未来将在多年冻土区修建大量机场, 这些机场的修建将不能避免多年冻土问题. 国内关于冻土区机场跑道修筑的经验非常有限, 国外则开始的较早, 并积累了一些经验. 总结分析国内外多年冻土区机场跑道修筑技术的现状, 其跑道类型主要有: 基岩跑道、开挖换填法修筑的跑道、铺设隔热层的跑道、安装热管的跑道, 共4类. 由于我国多年冻土区的特殊性, 国外的跑道修筑经验只能在一定程度上参考. 由于飞机跑道不同于铁(公)路的特殊性, 近年国内在冻土区铁(公)路的修建过程中采用的稳定冻土地基的工程措施如何应用到机场跑道的建设上, 仍需进一步研究、验证和实践. 将来在我国多年冻土区修建机场跑道, 应结合国外已有的技术和经验, 并以我国在多年冻土区线性工程中已取得的经验作为基础, 进一步研究我国多年冻土区机场跑道修筑的关键技术.     

青藏公路下伏多年冻土的融化分析

基于青藏公路沿线高温冻土区和低温冻土区2组地温观测孔5 a的地温观测资料, 研究了路基下伏多年冻土的融化状态, 定量分析了进入路基下多年冻土内的热状况. 结果表明: 路基近地表地温明显高于对应天然地表下的地温, 路基近地表经历的融化期长于对应天然地表, 高温冻土区路基内已形成贯穿融化夹层;进入高温冻土区路基下伏多年冻土内的热收支处于持续不断的吸热状态, 进入低温多年冻土区的热收支也呈现出吸热明显大于放热的周期性变化;高温冻土区接近0℃的地温及其持续不断的热积累是引起下伏多年冻土不断融化的主要原因. 低温冻土区进入多年冻土的热积累暂时以增高地温耗热为主, 随着地温的增高, 低温冻土区也可能发生强烈的冻土融化.     

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.