非最大融化深度季节多年冻土天然上限的确定方法

准确确定高纬度地区多年冻土的天然上限深度及其变化规律对于冻土地区铁路工程的设计和施工至关重要。传统现场勘探测温的方法,虽然比较准确,却有很大的时间限制,在非最大融化深度季节无法确定多年冻土的天然上限深度。为了能够在任何勘测季节都可以获得多年冻土的天然上限资料,本文在对大兴安岭多年冻土地区的多年勘测、测温资料的分析研究基础之上,总结推导出了4种比较行之有效的计算多年冻土天然上限的方法,对于快速而准确的确定多年冻土天然上限具有很好的指导作用。     

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.     

探地雷达在祁连山多年冻土调查中的应用

探地雷达用于多年冻_十区的勘测一般通过钻孔和探坑进行直接对比来确定冻土层分布状况,但在野外工作中,钻孔资料一般很难得到,而探坑在有限的人力物力条件下也很难开挖,这给冻土层的野外确定带来很大困难.我们采用雷达探测资料寻找浅层地下冰深度来确定多年冻土上限的深度,企图能在没有现场对比资料的情况下寻找一种利用探地雷达探测多年冻土的简易方法.探测结果显示,通过地貌特征寻找浅层地下冰可能存在的典型地段进行雷达探测能很容易确定多年冻上上限的位置.2007年在祁连山区利用Pulsc EKKO Pro探地雷达进行了多年冻土的野外探测,结果显示:大雪山老虎沟海拔3 684 m(39.5907°N;96.4339°E)处多年冻土上限约为2.2 m,在冷龙岭北坡的水管河源头海拔4 053 m(37.5463°N;101.7709°E)至海拔3 907 m(37.5508°N;101.7752°E)处的多年冻土上限深度为2.5 m,在宁昌河源头沿河岸从海拔3 448 m(37.5649°N;101.84 55°E)至海拔3 377 m(37.5797°N,101.8377°E)处多年冻土上限为2.4 m,在走廊南山的观山河源头海拔3 468 m(39.2615°N;98.6715°E)处多年冻土上限深度在2 m左右.另外根据4个勘察区多年冻土特征地貌分布区的最低分布海拔总结得出,老虎沟地区为冻土下界分布最高地区,关山河源头为冻土下界分布最低地区.其原因主要是降水和植被的差异造成的结果,降水量大和植被良好的地区多年冻土下界的分布海拔就低,反之亦然.     

影响多年冻土上限变化的因素探讨

利用地温及活动层水热观测资料,分析青藏公路沿线近年来影响多年冻土上限的变化因素.研究结果显示,青藏公路沿线冻土上限总体呈现下降趋势,冻土上限的变化与近年来区域气候变化的趋势一致;近年来多年冻土上限下降0.1～0.5 m,所处的地理位置不同,冻土上限下降的幅度也不同.气温变化是影响冻土上限的一个重要的外部因素,上限变化的...     

青藏铁路北麓河试验段冻土工程地质特征及评价

冻土问题是青藏铁路建设的难题之一,为良好的解决这一问题,详细了解线路通过地区的冻土工程地质特征并对其做出工程地质评价至关重要.在目前完成的青藏铁路北麓河试验段的冻土勘察工作表明,该试验段的土层以富含厚层地下冰的细粒土为主,试验段地下水丰富,全段高温与低温多年冻土都有分布,冻土上限深度一般为2～3m.综合上述特征,该试验段综合评价为不良和极差冻土工程地质地段.在类似地区进行铁路建设,工程措施设计和采用中要充分考虑冻土工程地质特征,否则可能导致工程建设的隐患甚至所采取工程措施的失败.     

214国道沿线的多年冻土及其工程地质条件评价

214国道位于青藏高原的东缘,1985-2012年期间的冻土勘察和地温监测资料表明,在河卡山至清水河439 km范围内的高山、滩地和沼泽化草甸地区分布着不连续和岛状多年冻土,公路实际穿越的多年冻土段累计里程约232.4 km,沿线绝大部分路段的地温高于-1.5℃,含冰量、冻土上限等多年冻土特征指标随地形、地貌变化剧烈. 在分析上述资料的基础上,从冻土热稳定性和自然环境两个因素入手,采用突变级数法建立了多年冻土工程地质条件评价模型并对214国道多年冻土工程地质条件进行了定量评价. 结果表明：214国道沿线冻土热稳定性普遍较差,自然环境多处于一般状态. 除局部少冰、多冰冻土路段以外,沿线多年冻土工程地质条件总体处于较差或恶劣状态. 与214国道病害调查资料进行比较后发现,路基病害一般发生在工程地质条件差的路段. 这表明该评价结果比较准确的反映了沿线的多年冻土工程地质条件,对于现有214国道和新建共和-玉树高速公路的运营和维护具有重要的指导意义.     

应用探地雷达研究中国小兴安岭地区黑河北安公路沿线岛状多年冻土的分布及其变化

结合探地雷达对我国东北黑大公路黑北段岛状多年冻土的勘察结果进行了应用分析研究. 结果表明, 探地雷达可以较为有效确定多年冻土分布区域、 厚层地下冰存在位置, 是研究多年冻土的一种有效手段. 探地雷达勘测结果表明, 东北小兴安岭岛状多年冻土现在主要位于山间沟谷洼地、 或山间盆地中, 地表有积水、 塔头草生长茂盛、 草炭和泥炭发育的沼泽化湿地是其存在的重要标志;结合20世纪70年代对该区的冻土调查结果, 以及线路沿线现存冻土比例推断, 在过去30 a间小兴安岭岛状多年冻土发生了较为显著的退化;现存黑河北安公路沿线稀疏岛状多年冻土区的比例约为2%, 冻土厚度约2～9 m, 冻土上限约1～3 m. 在影响多年冻土分布的因素中, 地表水分条件是最为关键的因素, 该地表水分通过蒸发吸热、 单向导热等作用调节地中热流, 并维持一定的净放热, 在年平均气温接近0 ℃的条件下仍可以维持冻土的发育和存在;其它影响因素, 如地形、 地貌、 坡向、 植被、 地质条件等因素发挥次要作用.     

北极多年冻土区埋地输气管道周边温度场数值分析

以北极规划输气管道工程为依托,建立埋地管道与冻土热交换相互作用数值计算模型,探究了埋地管道在连续多年冻土区、非连续多年冻土区和季节冻土区内,按照不同操作温度(5、-1和-5℃)运行情况下管道周围冻土温度演化过程.计算结果表明:同一区域不同管温对冻土上限值影响差异较大,尤其是在非连续多年冻土区,无论管道是正温输送还是负温输送,由于管道的运营,极大地影响了冻土上限值.5℃正温管道将导致冻土上限下降1～3倍管径;-1℃和-5℃负温管道将有助于提高冻土人为上限.建议在连续多年冻土区管道采用-1℃输送温度;在非连续多年冻土区冬季采用-1℃输送温度,夏季可以是正温,接近环境大气温度,但全年输气平均温度要小于0℃;在季节冻土区,若按照负温输送,反而容易引起管基土冻胀,建议输气温度不作特别控制,与温带地区管道类似,正温输送.希望能够为北极多年冻土区天然气管道建设提供新的思路.     

青藏公路路基变形分析

为研究青藏公路多年冻土人为上限在退化过程中对路基变形产生的影响过程和程度, 在唐古拉山以南选择了3处具有代表性的路面进行了为期2 a的路面变形观测. 资料表明, 在多年冻土人为上限退化过程中随着公路路基结构、冻土类型的不同, 路基变形从冻胀和融沉过程、冻胀量和融沉量、发生的时间都有很大的不同. 在高含冰量多年冻土区采用半挖半填结构产生的路基变形最为剧烈, 在含冰量相对少且采用较高路堤结构的地段路基变形过程相对平缓. 同时结合探地雷达的勘察结果对路基下的融化区、多年冻土区的内部结构进行了分析. 结果显示,多年冻土人为上限的下移、地下冰的融化会在多年冻土人为上限以上的地质体中导致较强烈的层间错动和扰动.     

中子水分计在多年冻土研究和工程中的应用

一、引言 在多年冻土地区,随着土中水分的冻结和融化,会导致一系列奇异独特的冻土现象,如冻胀丘、冻融滑塌和热融沉陷等。这些现象往往给结构物造成灾害,如建筑物的损坏,道路的翻浆和沉陷,管道的折裂和变形等。因此测定冻土水分随季节、土质和土层深度等的变化,确定冻结和融化速率及多年冻土上限等,就是冻土研究和勘测的一项重要内容。     

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.