长庆油田小套管二次固井工艺技术研究与应用

针对长庆油田?139.7 mm生产套管中下?88.9 mm小套管二次固井环空间隙小、固井施工压力高,水泥环薄、密封完整性难以满足后期措施需求,固井前井筒界面环境差、二界面水泥胶结不佳等技术难点,通过技术创新及改进,研制出适用于小套管二次固井的低摩阻耐压防漏水泥浆体系、热固性树脂水泥浆体系,结合自主研发的界面增强型冲洗液和固井压塞液体系,形成一套长庆油田小套管固井工作液体系。优选性能可靠的固井配套工具,优化小套管固井管串结构,按照平衡压力固井原理,采用一次上返固井工艺,总结出了一套小套管二次固井工艺技术。现场应用10口井,固井质量优良率95%,增产效果显著,为长庆油田老井增潜挖效及套损井治理提供了有力的技术支撑。     

一种遥感蚀变提取方法在地质找矿中的应用

正目前国内外遥感蚀变信息提取主要采用比值法、主成分分析法、光谱角法(田淑芳等,2013),在对蚀变分量进行阈值分割时大多使用基于统计学模型的门限化方法(Zhang Yujun et al., 2007),然而掩膜后的区域会使得统计参数产生偏移,当数据不服从正态分布时,提取的蚀变信息会存在较大误差。     

内蒙古水泉沟地区化探次生晕找矿效果浅析

水泉沟矿区在找矿初期,开展了1∶1万次生晕地球化学测量扫面工作。通过对该区异常的分析、筛选、野外地表检查、评价,圈定综合异常4处。为了对综合异常成因进一步的了解,对矿区圈定的异常区重点地段进一步开展了大比例尺(1∶2000)次生晕和地质综合剖面测量,详细的分解和解剖了异常地质成因,明确了区内的找矿方向,选定了下一步找矿靶区,为该区地质找矿工作提供了可靠的基础性化探资料。利用槽探对优选靶区异常进行地表查证,采用钻探工程对靶区槽探查证发现的矿体深部进行揭露,扩大了矿体规模。截至目前已发现多条工业矿体,增加了资源储量。充分证明了次生晕地球化学找矿方法在该区效果显著。     

基于ArcObjects的广州地铁售票系统设计与开发

选用了ArcObjects组件结合.NET平台,进行了GIS二次开发,整合了售票业务流程与地理导航功能。     

Numerical modelling of multiphase immiscible flow in double‐porosity featured groundwater systems

A numerical model describing the flow of multiphase, immiscible fluids in a deformable, double‐porosity featured soil has been developed. The model is focused on the modelling of the secondary porosity features in soil, which is more relevant to groundwater contamination problems. The non‐linear saturation and relative permeabilities were expressed as functions of the capillary pressures. The governing partial differential equations in terms of soil displacement and fluid pressures were solved numerically. Galerkin's weighted‐residual finite element method was employed to obtain the spatial discretization whereas temporal discretization was achieved using a fully implicit scheme. The model was verified against established, peer‐reviewed works, and the assumption that the immiscible fluids (non‐aqueous phase liquids) will flow preferentially through the secondary porosity features in soil was validated. Copyright © 2011 John Wiley & Sons, Ltd.     

关中平原大地等效电导率的间接测量

为准确预报地波传播时延,用电波传播法对关中平原的大地等效电导率进行了间接测量。阐述了电波传播法的测量原理和方法,第一次给出关中平原大地等效电导率的间接测量结果,同时,给出了中国科学院国家授时中心临潼科研楼参考点的BPL信号传播时延测量结果,并对这些测量结果进行了精度分析。     

Role of atmospheric ammonia in the formation of inorganic secondary particulate matter: A study at Kanpur,India

Levels of fine Particulate Matter (PM_fine), SO₂ and NO_x are interlinked through atmospheric reactions to a large extent. NO_x, NH₃, SO₂, temperature and humidity are the important atmospheric constituents/conditions governing formation of fine particulate sulfates and nitrates. To understand the formation of inorganic secondary particles (nitrates and sulfates) in the atmosphere, a study was undertaken in Kanpur, India. Specifically, the study was designed to measure the atmospheric levels of covering winter and summer seasons and day and night samplings to capture the diurnal variations. Results showed are found to be significantly high in winter season compared to the summer season. In winter, the molar ratio of to was found to be greater than 2:1. This higher molar ratio suggests that in addition to (NH₄)₂SO₄, NH₄NO₃ will be formed because of excess quantity of present. In summer, the molar ratio was less than 2:1 indicating deficit of to produce NH₄NO₃. The nitrogen conversion ratio (NO₂ to NO₃) was found to be nearly 50% in the study area that suggested quick conversion of NO₂ into nitric acid. As an overall conclusion, this study finds that NH₃ plays a vital role in the formation of fine inorganic secondary particles particularly so in winter months and there is a need to identify and assess sources of ammonia emissions in India.     

中国南海软珊瑚附生真菌Acremonium sp. SCSIO41216的次级代谢产物研究

采用硅胶柱层析色谱法、中压正相柱层析色谱法、中压反相柱层析色谱法以及半制备高效液相色谱法对中国南海软珊瑚来源真菌Acremonium sp. SCSIO41216的大米发酵产物进行分离纯化, 并使用核磁共振、质谱等波谱学方法, 结合其理化性质及文献数据鉴定了7个单体化合物结构: fischexanthone(1)、sydowinin A (2)、(22E)-5α,8α-epidioxyergosta-6,22-dien-3β-ol (3)、16-O-去乙酰基夫西地酸内酯(4)、环-(S)-脯氨酸-(R)-亮氨酸(5)、环-(S)-脯氨酸-8-羟基-(R)-异亮氨酸(6)和环(L)-脯氨酸-(L)-苯丙氨酸(7)。化合物1—7均首次从海洋软珊瑚来源的枝顶孢属真菌(Acremonium sp.)中分离获得。     

Do young martian ray craters have ages consistent with the crater count system?

McEwen et al. (McEwen, A.S., Preblich, B.S., Turtle, E.P., Artemieva, N.A., Golombek, M.P., Hurst, M., Kirk, R.L., Burr, D.M., Christensen, P. [2005]. Icarus 176, 351-381) developed a useful test for the internal consistency of crater-count chronometry systems. They argued that certain multi-kilometer, fresh-looking martian craters with prominent rays should be the youngest or near-youngest craters in their size range. The “McEwen et al. test” is that the ages determined from crater densities of the smallest superimposed craters (typically diameter D ∼ 5-20 m) should thus be comparable to the expected formation intervals of the host primary. McEwen et al. concluded from MOC data that crater chronometry failed this test by factors of 700-2000. We apply HiRISE and other imagery to eight different young craters in order to re-evaluate their arguments. We use existing crater chronology systems as well as the reported observed production rate of 16 m craters (Malin, M.C., Edgett, K., Posiolova, L., McColley, S., Noe Dobrea, E. [2006]. Science 314, 1573-1557; Hartmann, W.K., Quantin, C., Mangold, N. [2007]. Icarus 186, 11-23; Kreslavsky [2007]. Seventh International Conference on Mars, 3325). Every case passes the McEwen et al. test. We conclude that the huge inconsistencies suggested by McEwen et al. are spurious. Many of these craters show evidence of impact into ice-rich material, and appear to have ice-flow features and sublimation pits on their floors. As production rate data improve, decameter-scale craters will provide a valuable way of dating these young martian geological formations and the processes that modify them.     

基于MAPGIS二次开发的采矿权登记信息自动矢量化

以MAPGIS6.7为平台,结合VB6.0和ACEESS数据库进行二次开发,实现了采矿权登记信息数据库精确、快速的自动矢量化,为矿山遥感调查与监测项目提供了强有力的技术支持,有效提高了实际工作效率。