穿越采空区氮气钻井工艺应用研究

以寺河矿区穿越采空区氮气钻井试验为背景,通过分析煤层取心测试数据,指出钻井穿越3号煤层采空区抽采9+15号煤层瓦斯的必要性。利用“三带”理论明确了3号煤层采空区顶板以上74.4 m及底板以下22.73 m为钻井漏失带,采用氮气钻井穿越该层段有助于安全高效施工;优化了穿越采空区氮气钻井的三开井身结构;根据穿越采空区氮气钻井工艺需要,配套设计了地面钻井工艺流程。氮气钻井工艺在寺河矿区试验的成功,证明该工艺的可行性,对穿越采空区钻井技术的研究和推广应用具有重要的指导意义。     

在某污染的工业废物填埋场环境水文 地质评价中的同位素水文学研究

本文论述了某污染的工业废物填埋场场址的地质、水文地质条件,应用水化学方法、环境同位素技术(地下水中氚及氢、氧稳定同位素)和同位素单孔示踪技术等同位素水文学领域中的新方法对区内地下水的活动条件以及填埋场场址区分布的第四系孔隙潜水和第三纪红层孔隙-裂隙水的成因进行了分析,测量并确定了填埋场下部地下水的流速及流向。研究结果表明场区地下水的运动与地表水无直接水力联系。污染的工业废物填埋后不会通过地下水的迁移造成对地表水的污染,进而证实填埋场的地质、水文地质条件对处置污染的工业废物是安全可靠的。     

基于PSO-PP的围岩稳定性评价

围岩的稳定性评价是一个复杂的不确定系统问题。结合投影寻踪方法、粒子群算法和逻辑斯谛曲线函数,建立了围岩稳定性评价的粒子群优化投影寻踪(projection pursuit based on particle swarm optimization,PSO-PP)模型。该模型一方面采用粒子群算法优化投影指标函数及逻辑斯谛曲线函数参数,确保了模型的准确性;另一方面利用逻辑斯谛曲线函数建立投影值与经验等级之间的非线性关系。模型的测试结果显示了良好的精度,实例分析结果与实际状态完全一致,表明该模型在围岩稳定性评价中的可行性和有效性。     

福建邵武地区大坪—张厝一带萤石矿地质特征及下一步工作方向

正研究区位于福建省邵武市大坪—张厝一带,区内断裂构造发育,萤石矿化强烈,物化探异常明显,萤石矿床(点)众多。综合区内成矿地质特征及成矿规律,区内萤石矿找矿潜力大,新发现的张厝、新坪萤石矿通过进一步工作,有望达到中大型萤石矿床规模。1 区域地质     

东昆仑东段布青山地区上二叠统格曲组物源分析及其构造意义

对东昆仑东段布青山得力斯坦地区出露的上二叠统格曲组砾岩层进行砾石成分、砾度统计及系统的LA-ICP-MS锆石UPb年龄谱分析。结果表明,格曲组砾岩层砾石成分以石英岩和花岗岩为主,硅质岩和基性岩次之,砂岩和灰岩较少,砾石的分散系数为1.54~2.02,该套砾岩为近源快速堆积的产物。砾岩碎屑锆石U-Pb年龄可分为3组:1早奥陶世—晚志留世年龄组为499~409Ma,峰值年龄为426Ma,对应早古生代末期原特提斯洋向北俯冲碰撞产生的一系列构造岩浆事件;2新元古代年龄组为744~619Ma,峰值年龄为744Ma,对应于全球Rodinia超大陆裂解事件;3古元古代年龄组为2443Ma,对应东昆仑地区古元古代构造岩浆热事件。结合碎屑锆石年龄及沉积学特征综合分析,花岗质砾石来源于北侧东昆仑造山带加里东期岩浆弧,沉积岩砾石则可能来自造山带早期的沉积地层,石英岩及其他变质岩砾石则多来自东昆仑基底变质岩系。综合判别,格曲组为一套沉积于活动大陆边缘环境的滨浅海相磨拉石建造,代表南侧古特提斯洋向北俯冲开始的构造阶段,是初始俯冲的沉积构造响应。     

A numerical study on the role of atmospheric forcing on mixed layer depth variability in the Bay of Bengal using a regional ocean model

Ocean Dynamics - This study investigates the role of driving atmospheric forces [winds, net heat flux, and evaporation–precipitation (E–P)] and the possible mechanisms on the mixed...     

Rapid earthquake hazard and loss assessment for Euro-Mediterranean region

The almost-real time estimation of ground shaking and losses after a major earthquake in the Euro-Mediterranean region was performed in the framework of the Joint Research Activity 3 (JRA-3) component of the EU FP6 Project entitled “Network of Research Infra-structures for European Seismology, NERIES”. This project consists of finding the most likely location of the earthquake source by estimating the fault rupture parameters on the basis of rapid inversion of data from on-line regional broadband stations. It also includes an estimation of the spatial distribution of selected site-specific ground motion parameters at engineering bedrock through region-specific ground motion prediction equations (GMPEs) or physical simulation of ground motion. By using the Earthquake Loss Estimation Routine (ELER) software, the multi-level methodology developed for real time estimation of losses is capable of incorporating regional variability and sources of uncertainty stemming from GMPEs, fault finiteness, site modifications, inventory of physical and social elements subjected to earthquake hazard and the associated vulnerability relationships.     

Atmospheric Surface-Layer Processes During the Total Solar Eclipse Of 11 August 1999

The central path of the total solar eclipse (TSE) of 11 August 1999 mostly passedthrough a region of active monsoon in India, with the eclipse ending around localsunset. Measurements in the surface layer (SL) were carried out close to the eclipseaxis at Akola (20°42' N, 77°2' E) in central India. The globalradiation flux reaching the surface vanishes around totality at 1803:24 (LT), followedby a small recovery before again dipping to zero at sunset. The temperatures in the SL, and subsoil at 50-mm depth, show a local minimum with a lag of about 10 min after the second contact, whereas the lag appears to vanish when the temperature series is detrended. The SL exhibits near-neutral, though generally stable, conditions from about 1500 hr itself due to heavy cloud cover followed by the eclipse-induced cooling of the surface. The wind component across the eclipse axis vanishes at totality, the wind vector aligning with the azimuth of the traversing moon shadow. The deceleration of the mean flow can be due to the combined effect of the colder surface and downward heat flux, where the locally altered horizontal temperature gradients may cause, as in this instance, the cessation of the cross flow.The oscillations in temperature and wind that show significant peaks, around 90–100 min as well as the semi-period of the eclipse near 60 min, persist for several hours past the eclipse event. A fresh analysis of the published data on the TSE of 7 March 1970 shows spectral peaks in the temperature nearly coincident with those already reported from the surface pressure records. The oscillations in the SL fields during the two TSE events are very similar implying that the source mechanism is also likely to be the same in both the cases.     

盆东伏旱气候的时空分布及其形成原因

利用盆东地区气象、水文及其它专业部门的共403个测站的雨量、气温等基本气象资料,分析了盆东气候区大春生长季节的基本气候特点及其形成原因.针对盆东多山的具体情况,分析中突出了山地立体气体特色,进一步查明了盆东农业气候资源,为因地制宜进行农业现代化建设,提供了气象科学数据.     

Simulation of the annual and diurnal cycles of rainfall over South Africa by a regional climate model

The capability of a current state-of-the-art regional climate model for simulating the diurnal and annual cycles of rainfall over a complex subtropical region is documented here. Hourly rainfall is simulated over Southern Africa for 1998–2006 by the non-hydrostatic model weather research and forecasting (WRF), and compared to a network of 103 stations covering South Africa. We used five simulations, four of which consist of different parameterizations for atmospheric convection at a 0.5 × 0.5° resolution, performed to test the physic-dependency of the results. The fifth experiment uses explicit convection over tropical South Africa at a 1/30° resolution. WRF simulates realistic mean rainfall fields, albeit wet biases over tropical Africa. The model mean biases are strongly modulated by the convective scheme used for the simulations. The annual cycle of rainfall is well simulated over South Africa, mostly influenced by tropical summer rainfall except in the Western Cape region experiencing winter rainfall. The diurnal cycle shows a timing bias, with atmospheric convection occurring too early in the afternoon, and causing too abundant rainfall. This result, particularly true in summer over the northeastern part of the country, is weakly physic-dependent. Cloud-resolving simulations do not clearly reduce the diurnal cycle biases. In the end, the rainfall overestimations appear to be mostly imputable to the afternoon hours of the austral summer rainy season, i.e., the periods during which convective activity is intense over the region.