人工边坡潜在滑动面研究——以广州科学城某人工高边坡为例   总被引：2，自引：2，他引：0  

徐佩华  陈剑平  石丙飞  仲志成 《吉林大学学报(地球科学版)》2008,38(5)

运用强度参数的改变对边坡破坏面形迹影响不明显这一特点,在数值模拟过程中通过改变岩体强度参数,有效地获取潜在滑动面的位置和形态,较好地解决了滑动面搜索的难题。将该法应用于广州科学城某人工高边坡稳定性的研究,在三维数值模拟过程中,将强度参数大幅度折减,计算后获得各剖面的剪应变增量图,从这些图中可获得潜在滑动面。这与人们通常将此类边坡的中风化面作为滑动面存在较大差别。将该滑动面运用极限平衡法进行计算,计算结果显示各剖面的安全系数基本都大于1.2,边坡稳定但仍需要加固处理,与三维数值模拟结果相一致。由此认为用这种分析法确定出的潜在滑动面合理、计算结果可靠,可作为搜索边坡潜在滑动面并计算安全系数的方法之一。  相似文献   

非均匀月壤介质的被动微波辐射传输模拟   总被引：1，自引：1，他引：0  

孟治国  陈圣波  刘财  杜晓娟  吕航 《吉林大学学报(地球科学版)》2008,38(6)

基于非均匀月壤物理模型和辐射传输方程,模拟月壤介质中的微波辐射传输特性,探讨频率、月壤厚度等与月表亮温的关系。结果表明:在低频段,月壤微波辐射亮温的动态变化范围较大,可探测的月壤厚度大,3 GHz时的最大可探测月壤厚度达12.4 m;在高频段对应的可探测月壤厚度较小,特别是从50GHz往后的频率段内,最大可探测月壤厚度均小于2 m。不同频率的亮温-厚度变化曲线没有交叉点,且频率越高,所能探测的月壤厚度越小。根据模拟结果,建立了月壤厚度与亮温的查找表。基于查找表,利用单个波段的亮温数据即可得到月壤厚度信息。  相似文献   

贵州糯东井田水文地质条件分析     

李军 《中国煤炭地质》2008,20(4):44-48

通过对井田内泉和暗河流量的调查研究,认为永宁镇组一、三段碳酸盐岩裂隙溶洞水为井田的主要含水层,含水层主要接受大气降水及河流的渗透补给;煤层上覆地层飞仙关组为相对隔水层,厚度大于500m,下覆无强含水层,其地下水对煤层的开采影响不大,井田水文地质条件较简单。采用比拟法对井田的涌水量进行了预算,推算该矿井开采设计涌水量为13 238m^3/d。  相似文献   

临涣矿区界沟煤矿工程地质条件研究     

黄芳友  张文永  徐胜平 《中国煤炭地质》2008,(7):55-58

根据主采煤层顶底板岩体岩性类型及结构面发育程度对其稳定性进行了评价：72煤层顶板以中等稳定一不稳定类型为主,82煤层顶板以中等稳定类型为主,10煤层顶板以中等稳定一稳定类型为主。在大量统计见煤点硬质岩百分含量（k值）的基础上,结合顶板岩石的单轴抗压强度,对各主采煤层顶底板工程地质类型进行了划分：72煤层以一、二类顶板为主,82、10煤层均以五类顶板为主。综合评价该矿工程地质条件为中等即Ⅲ类二型。根据研究成果,指出该矿在采掘过程中可能出现的工程地质问题,并依此提出了治理建议。  相似文献   

三维地震技术在煤层顶板稳定性研究中的应用     

孙立新  许崇宝  王真 《中国煤炭地质》2008,(11):55-57

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   

数值模拟技术在海坨子油田开发调整研究中的应用     

翟雨阳  刘钦甫  张立德  唐勇  刘振兴 《上海国土资源》2008,(2):47-50

讨论分析数值模拟技术在海坨子油田开发调整研究中的思路和方法,采用美国Landmark公司VIP2003．4版本数值模拟软件包进行模拟研究,通过参数准备,静、动态拟合,模拟出海坨子油田海S9—11井组1—9砂组各小层剩余储量大小及不同阶段流体饱和度分布,结合可视化技术形象描述了海坨子油田剩余油变化规律及潜力区,在此基础上预测不同井网加密方式开发指标,并优选出最佳方案,为海坨子油田下步开发调整提供了重要依据,取得了较好的效果。  相似文献   

CSU－RAMS模式在区域气侯模拟中的应用   总被引：1，自引：0，他引：1  

万齐林  施永年 《热带气象学报》1996,(2)

将ＣＳＵ－ＲＡＭＳ（中尺度）数值模式改造成“区域气候数值模式”以及进行区域气候数值模拟的试验研究。说明将有限区域中尺度数值模式与ＧＣＭ模式嵌套应用到区域气候数值模拟研究上能够取得有意义的结果。它能在一定程度上改善ＧＣＭ模式的不足。可以更为细致地描述大气环流的变化特征,是了解区域气候变化的有效方法之一。  相似文献   

Information structure analysis for quantitative assessment of mineral resources and the discovery of a silver deposit     

Wang  Yutian  Tan  Bingqi  Wang  Yifeng  Wu  Jiangtao 《Natural Resources Research》1994,3(4):284-294

We propose an information-structure-analysis (ISA) method to quantify the correlations between quantitative and qualitative variables as well as within each type of variable. This method is applied to the evaluation of mineral resources in the western Zheijiang Province of China. The district contains a number of silver-bearing Fe–Cu–Pb–Zn mineral deposits near igneous complexes and FeCuPbZn zones away from the complexes. Silver anomalies occur not only in the known Fe–Cu–Zn–Pb deposits, but also in the country rock, suggesting the possible existence of silver deposits far from the igneous complexes.The tonnage distribution of silver is modeled by Monte Carlo simulation. This simulation is conducted on the basis of the correlations between silver (Ag) and lead (Pb), since no known data on silver is available. The known tonnage distribution of lead in 11 control cells was used to approximate the tonnage distribution of silver in the Monte Carlo simulation. With ISA and Monte Carlo methods, the total amount of potential polymetallic resources in 49 cells in the western Zhejiang Provice is predicted. Significantly, a deposit with about 24 tonnes of silver has been found within our exploration target area.  相似文献   

Periodic orbits and their bifurcations in a 3-D system     

G. Contopoulos  B. Barbanis 《Celestial Mechanics and Dynamical Astronomy》1994,59(3):279-300

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   

Effect of perturbed potentials on the non-linear stability of libration pointL 4 in the restricted problem     

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:

(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.

  相似文献