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61.
浅埋双连拱隧道围岩边坡体系变形机理及稳定性分析 总被引:2,自引:0,他引:2
双连拱隧道是一种新的隧道形式, 由于其整体跨度大、结构复杂、施工工序繁琐, 在地形偏压、地质条件复杂的情况下修建双连拱隧道难度较高, 尤其在洞口段容易出现衬砌开裂、边坡变形等一系列工程问题。结合安徽铜黄高速公路汤屯段富溪隧道进口段工程, 采用地质条件研究与数值模拟分析相结合的研究手段, 对复杂地质条件下偏压双连拱隧道围岩① 边坡体系在施工过程中应力应变发展过程进行了研究。综合分析表明, 富溪隧道进口段处于F5断层影响带内, 岩体呈碎裂结构,同时, 受到地形偏压影响, 隧道开挖后衬砌和围岩表现为沉降变形和侧向变形, 进口边坡在隧道围岩变形的诱导下, 表现为蠕滑- 拉裂变形破裂。根据以上研究成果, 提出了富溪隧道变形治理应以控制进口段隧道拱顶的变形为主。 相似文献
62.
沪蓉高速柴家湾隧道围岩稳定性分析及支护效果研究 总被引:1,自引:0,他引:1
隧道围岩的应力分布及变形特征对保证其长期稳定性具有关键的作用。本文以柴家湾隧道为例进行实态建模,通过采用有限元软件ANSYS对其施工全过程进行了三维弹塑性数值模拟计算。研究结果表明,隧道拱顶和拱脚处应力集中现象明显,局部可能出现拉应力;变形主要集中在拱顶、拱腰部位,衬砌单元所受内力在规定强度范围以内,支护措施合理有效。 相似文献
63.
Slope inclinometers for landslides 总被引:2,自引:1,他引:1
Slope inclinometers/indicators are used to determine the magnitude, rate, direction, depth, and type of landslide movement.
This information is usually vitally important for understanding the cause, behavior, and remediation of a landslide. However,
many inclinometer measurements fail to achieve these intended aims because of lack of appreciation of the many factors that
need to be correctly implemented during installation, monitoring, and data reduction to yield useful data. This paper presents
some guidelines for understanding, installing, and interpreting slope inclinometers and presents three case histories that
illustrate some of the pitfalls that can develop if these guidelines are not followed. 相似文献
64.
均匀设计与灰色理论在边坡稳定性分析中的应用 总被引:1,自引:1,他引:0
采用均匀设计安排试验,运用灰色理论中的灰色关联分析考察边坡稳定性影响因素的主次.结果表明,边坡稳定性影响因素的敏感性由大到小依次为:粘聚力、内摩擦角、重度、预应力、锚索间排距、锚索长度、锚固段长度、锚固角.可见,岩体的抗剪强度指标是影响边坡稳定性的最重要参数,其次是岩体的容重,而预应力锚索的设计参数对边坡的稳定性也有一定影响.这一分析结果为边坡开挖设计和加固方案的优化提供了重要依据. 相似文献
65.
66.
龙固井田为全隐蔽的华北型煤田,位于巨野煤田中部,其首采扩大区主采煤层为3号煤层。考虑3煤层顶板稳定性主要受其顶板的构造信息和岩性信息影响,因此首先依据三维地震勘探综合解释成果及波阻抗反演解释成果对二者进行定量化,然后对波阻抗数据进行归一化处理,使得波阻抗数据和量化后的构造数据具有相同的变化范围及等量贡献。在此距离范围内构造和岩性的权值各为0.5,依此生成综合因素煤层顶板稳定性隶属度。分析3煤层顶板以上10m、20m处的综合因素煤层顶板稳定性隶属度图可以发现,该区3煤层顶板稳定性比较好。且其稳定性主要是受构造因素控制,岩性因素相对影响较小。 相似文献
67.
We study some simple periodic orbits and their bifurcations in the Hamiltonian
. We give the forms of the orbits, the characteristics of the main families, and some existence diagrams and stability diagrams. The existence diagram of the family 1a contains regions that are stable (S), simply unstable (U), doubly unstable (DU) and complex unstable (). In the regionsS andU there are lines of equal rotation numberm/n. Along these lines we have bifurcations of families of periodic orbits of multiplicityn. When these lines reach the boundary of the complex unstable region, they are tangent to it. Inside the region there are linesm/n, along which the orbits 1a, describedn-times, are doubly unstable; however, along these lines there are no bifurcations ofn-ple periodic orbits. The families bifurcating from 1a exist only in certain regions of the parameter space (, ). The limiting lines of these regions join at particular points representing collisions of bifurcations. These collisions of bifurcations produce a nonuniqueness of the various families of periodic orbits. The complicated structure of the various bifurcations can be understood by constructing appropriate stability diagrams. 相似文献
68.
K. B. Bhatnagar Usha Gupta Rashmi Bhardwaj 《Celestial Mechanics and Dynamical Astronomy》1994,59(4):345-374
The non-linear stability of the libration pointL
4 in the restricted problem has been studied when there are perturbations in the potentials between the bodies. It is seen that the pointL
4 is stable for all mass ratios in the range of linear stability except for three mass ratios depending upon the perturbing functions. The theory is applied to the following four cases:
相似文献
(i) | There are no perturbations in the potentials (classical problem). |
(ii) | Only the bigger primary is an oblate spheroid whose axis of symmetry is perpendicular to the plane of relative motion (circular) of the primaries. |
(iii) | Both the primaries are oblate spheroids whose axes of symmetry are perpendicular to the plane of relative motion (circular) of the primaries. |
(iv) | The primaries are spherical in shape and the bigger is a source of radiation. |
69.
Zuzanna Niedzielska 《Celestial Mechanics and Dynamical Astronomy》1994,58(3):203-213
The stability of the triangular libration points in the case when the first and the second order resonances appear was investigated. It was proved that the first order resonances do not cause instability. The second order resonances may lead to instability. Domains of the instability in the two-dimensional parameter space were determined. 相似文献
70.
A comparison is made between the stability criteria of Hill and that of Laplace to determine the stability of outer planetary orbits encircling binary stars. The restricted, analytically determined results of Hill's method by Szebehely and co-workers and the general, numerically integrated results of Laplace's method by Graziani and Black are compared for varying values of the mass parameter =m
2/(m
1+m
2). For 00.15, the closest orbit (lower limit of radius) an outer planet in a binary system can have and still remain stable is determined by Hill's stability criterion. For >0.15, the critical radius is determined by Laplace's stability criterion. It appears that the Graziani-Black stability criterion describes the critical orbit within a few percent for all values of . 相似文献