土质滑坡格构锚杆抗滑机制及受力试验研究     

韩冬冬  门玉明  胡兆江 《岩土力学》2020,41(4):1189-1194

通过滑坡防治格构锚固大型物理模型试验，分析了土质滑坡格构锚杆体系在坡顶荷载下的变形和位移，揭示了格构锚杆的抗滑机制，探讨了锚固力与坡体位移及锚杆变形的关系，提出了极限锚固力的计算方法。结果表明：滑坡滑动时，格构梁与坡体整体发生旋转滑移，锚杆在滑面处发生了弯曲变形，处于弯曲和轴向拉伸组合变形状态；格构锚杆的抗滑作用表现为锚杆在滑面处的抗剪抗滑和锚杆格构梁的挡土阻滑；格构锚杆的极限锚固力由初始预应力、锚杆弯曲变形引起锚拉力、坡体位移引起锚拉力三部分组成，可通过公式 计算。该研究结果可为格构锚固体系的优化设计提供一定的参考。  相似文献   

A simplified mathematical model for the dam-breach hydrograph for three reservoir geometries following a sudden full dam break     

Hu  Hui  Zhang  Jianfeng  Li  Tao  Yang  Jie 《Natural Hazards》2020,102(3):1515-1540

Natural Hazards - The prediction of dam-break water flow at dam site is essential to reduce the potential for loss of damage in the downstream floodplain. In this study, the influence of reservoir...  相似文献   

隧道工程地震易损性分析研究综述与展望          下载免费PDF全文

吴桥  程永志  黄超 《世界地震工程》2020,(2):191-199

易损性分析是隧道工程领域防震减灾研究的重要方法。首先,详细综述了国内外隧道地震易损性研究历史与现状;其次,归纳了国内外隧道地震易损性分析主要方法,并总结了各种方法的实际适用性;接着,提出了隧道地震易损性评估步骤,并且讨论了以数值模拟为主要手段的理论易损性曲线建立中的3个关键内容:(1)输入参数确定;(2)破坏状态分级;(3)相关不确定性参数计算;最后,指出该领域一些亟待解决的问题和未来研究发展的方向。结果表明:隧道地震易损性分析能通过考虑相关不确定性因素,反映了隧道在地震荷载作用下的性能,有利于未来的风险评估和损失估算,对基于性能的隧道抗震设计的发展具有重要意义。  相似文献   

Evaluation of urban underground space resources using a negative list method: Taking Xi’an City as an example in China     

《China Geology》2020,3(1):124-136

Utilization of urban underground space has become a vital approach to alleviate the strain on urban land resources, and to optimize the structure and pattem of the city. It is also very important to improve the city environment, build livable city and increase the capacity of the city. Based on the analysis of existing evaluation methods and their problems, a method for evaluating underground space resources based on a negative list of adverse factors affecting underground space development is proposed, to be primarily used in urban planning stages. A list of the adverse factors is established, including limiting factors, constraining factors and influencing factors. Taking Xi’an as an example, using a geographical information system platform, a negative list of adverse factors for the underground space resources in Xi’ an City are evaluated, and preventive measures are proposed. Natural resources, exploitable resources, and the potential growth of exploitable underground space resources are evaluated. Underground space assessment in the different development stages of the city, collaborative utilization and safety evaluation for multiple subsurface resources, environmental impact and assessment, as well as evaluation methods based on big data and intelligent optimization algorithms are all discussed with the aim of serving city planning and construction.  相似文献   

Precise Determination of Astronomical Azimuth by the Hour Angle Method of Multiple Meridian Stars     

《Chinese Astronomy and Astrophysics》2020,44(4):536-548

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近15a陕西省植被时空变化与影响因素分析          下载免费PDF全文

岳辉  刘英 《干旱区地理》2019,42(2):314-323

利用2000—2014年MODIS/NDVI时间序列数据，采用栅格像元趋势分析、稳定性评价的方法，研究了陕西省近15 a植被的时空变化特征和规律；利用Hurst指数对陕西省植被未来变化趋势进行了预测；并利用相关性分析法分析了NDVI与年均温度和降雨量的关系。结果表明，2000年、2015年陕西省NDVI均值分别为0.4273、0.4942， 15 a来增加了0.067，增长了16.0%，其中陕北地区NDVI增加明显，关中部分地区出现负增长，陕南地区NDVI总体依旧维持在较高水平。陕西省植被变化趋势具有明显的空间差异性，全省植被未变化的占52.0 %，改善部分占44.27 %，退化部分占3.73%，说明15 a间陕西省植被覆盖改善面积大于退化面积，植被状况有所改善；其中陕北地区植被呈明显改善区域面积较大，关中地区植被覆盖面积有所减少，陕南地区植被变化幅度较小。陕西省植被稳定区域占50%以上（0 0.2)，说明15a间陕西省植被较为稳定，变化程度不大；其中陕西省植被最稳定地区主要集中在陕南、延安南部，榆林部分、西安、渭南少部地区变化幅度较大。Hurst指数分析表明陕西省44.54%面积的植被未来有可能面临退化，主要分布在陕北和关中地区的北部，植被未来有可能退化也有可能改善的面积占49.78%，主要分布在延安和陕南地区。陕西省近15 a气温和降水量总体呈增加趋势，增加速率分别为0.48 ℃·(10 a)-1和69.5 mm ( a)-1；相关性分析结果表明，年均降雨量是影响NDVI的主要气象因子，同时陕西省植被变化也受到了退耕还林还草、防沙治沙、生态政治等人为因素的影响。  相似文献   

Fingerprinting hydrothermal fluids in porphyry Cu deposits using K and Mg isotopes     

Li  Weiqiang  Zhao  Shugao  Wang  Xiaomin  Li  Shilei  Wang  Guoguang  Yang  Tao  Jin  Zhangdong 《中国科学:地球科学(英文版)》2020,63(1):108-120

In this study, we performed an integrated investigation of K and Mg isotopes in hydrothermally altered rocks from the giant Dexing porphyry Cu deposit in China. Both the altered porphyry intrusion and the surrounding wall rocks exhibit large variations in K and Mg isotope compositions, with δ41K values ranging between-1.02‰ and 0.38‰, and δ26Mg values ranging between-0.49‰ and 0.32‰. The δ41K and δ26Mg values of the majority of altered samples are higher than the isotopic baseline values for upper continental crust. We attribute the general increase in δ41 K and δ26Mg in altered rocks to hydrothermal alteration,which caused preferential incorporation of heavy K and Mg isotopes in alteration products, particularly phyllosilicates. However,a few altered samples show anomalously low δ41K and δ26Mg values. The δ41K and δ26Mg values do not correlate with K and Mg concentrations, or mineralogy of altered samples. The variable K-Mg isotope data likely reflect fluids of different physicalchemical properties, or different isotopic compositions. Based on the combined K-Mg isotope data, at least three groups of hydrothermal fluids are distinguished from the Dexing porphyry deposit. Therefore, K-Mg isotopes are potentially a novel tracer for fingerprinting fluids in complex hydrothermal systems.  相似文献   

Formation of Carbon-Enhanced Metal-Poor RR Lyrae Stars     

《Chinese Astronomy and Astrophysics》2020,44(1):61-69

Carbon-enhanced metal-poor (CEMP) stars are considered to be related to the first generation of stars, and responsible for the chemical evolution of the early Galaxy. More than half of them are in binaries, and could be explained by the binary evolution, but the formation channel of them is still not fully understood. Among the hundreds of CEMP stars, there are nine CEMP RR Lyrae stars identified, and at least seven of which are very likely not binaries. The usual binary star evolution channel is difficult to produce such a single star, particularly that of carbon enrichment. One way in which such a single star might be produced is the merger of a helium white dwarf with a Hertzsprung gap (HG) star. We use a stellar evolution program to calculate the models of the merger remnants, and find that the models can reproduce the observed distribution of these CEMP single RR Lyrae stars in terms of surface temperature, gravity, and carbon abundance. Hence, it is extremely possible that the helium white dwarf and HG star merger model is one of the formation channels of the metal-poor carbon-rich RR Lyrae stars.  相似文献   

Research on the Methods of Performance Monitoring and Evaluation for Active Hydrogen Maserstwo     

《Chinese Astronomy and Astrophysics》2019,43(2):292-304

Active hydrogen maser is the main frequency standard for establishing and maintaining the time scale. It has the characteristics of high short-term stability and low phase noise. At present, it plays an increasingly important role in the international atomic time (TAI) and various local time scales. Firstly, in combination with the internal state parameters of an active hydrogen maser, the correlation between the internal state parameters and the comparison data of a hydrogen maser is analyzed, and a method for the performance monitoring of a hydrogen maser is proposed. Secondly, according to the characteristics of hydrogen maser performance, a method for evaluating the performance of a hydrogen maser is given. The hydrogen maser performance includes mainly two aspects, namely the frequency stability and predictability. The performances of two types of active hydrogen masers (CH1-75 and MHM-2010) are evaluated by this method. The correlation analysis of the atomic clock state parameters and comparison data shows that the state parameter monitoring can effectively predict the variation of the hydrogen maser performance. The evaluation results of atomic clock frequency stability and predictability show that the atomic clock with a higher medium-and-long term frequency stability has a better predictability. There are two methods for the predictability evaluation, one is based on the data published by BIPM (Bureau International des Poids et Measures), and another one is based on the quadratic model. Both methods are consistent with the weights published by BIPM. Therefore, the two methods can be used as a quantitative method to evaluate the predictability of a hydrogen maser.  相似文献   

Analysis and Comparison for Fusion Algorithms of Time Transfer     

WANG Wei-xiong  DONG Shao-wu  WU Wen-jun  GUO Dong  ZHANG Jian 《Chinese Astronomy and Astrophysics》2021,45(2):224-235

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