EH-4电磁成像系统在隐伏构造探测中的应用

EH-4电磁成像系统具有勘探深度大、反映成果直观、轻便高效等优点.本文介绍了EH-4电磁成像系统的基本原理、数据采集和数据处理方法,及其在云南西部探测构造深部延伸情况的应用.实践证明,EH-4技术在探测构造深部延伸的应用方面是有效的.     

武当地块与扬子陆核区新元古代早期沉积岩碎屑锆石U-Pb年代学对比及其地质意义

系统收集并总结了武当地块与扬子陆核区(崆岭地区)已发表的新元古代沉积岩中碎屑锆石的U-Pb年代学数据,对二者的相互关系进行分析,并讨论了扬子克拉通北缘新元古代时期的构造演化过程及特征。对前人发表的年代学数据进行的统计和对比结果表明,武当地块沉积岩中碎屑锆石年龄谱记录了~710Ma和~2.5Ga的年龄峰值,同时缺乏3.0Ga年龄的锆石,表明其沉积物质来源可能并非扬子陆核区,其在新元古代之前可能作为一个独立的微陆块与扬子陆核区(崆岭地区)分离开来,二者于新元古代中期发生碰撞拼合而成为一个整体。     

基于LA-ICP-MS多元素成像技术的早寒武世磷结核成因研究

我国下寒武统底部广泛发育磷结核、磷块岩等富磷沉积,为早寒武世最为重要的化学标志层之一,也代表了隐生宙—显生宙转折期地球表层系统的重大变革。当前对磷来源和富集机制的解释不一。为进一步明确该时期富磷沉积的形成机制,本文利用激光剥蚀电感耦合等离子体质谱联用技术(LA-ICP-MS)对贵州金沙地区牛蹄塘组黑色页岩中的磷结核进行多元素原位微区成像研究。结果表明:磷结核中各元素富集情况清晰地记录了磷结核形成过程中微环境的变化趋势。其中,磷结核内部Ca、P共富集以及Si亏损,指示P富集缘于自生磷灰石生成,P则来自于有机质含氧或厌氧降解释放;Mn、Zn与P共富集于磷结核内部,指示结核形成时的底部水体为含氧水体;As、Mo、V等元素主要富集于围岩或黑色页岩,指示缺氧含H_2S水体形成终止了结核生长。本研究显示,LA-ICP-MS原位多元素成像技术能够获取微区内丰富的地球化学信息,并提供高精度可视化证据,未来将在地质勘探和古环境研究等领域得到更广泛应用。     

X-ray computed tomography of planetary materials: A primer and review of recent studies

X-ray computed tomography (XCT) is a powerful 3D imaging technique that has been used to investigate meteorites, mission-returned samples, and other planetary materials of all scales from dust particles to large rocks. With this technique, a 3D volume representing the X-ray attenuation (which is sensitive to composition and density) of the materials within an object is produced, allowing various components and textures to be observed and quantified. As with any analytical technique, a thorough understanding of the underlying physical principles, system components, and data acquisition parameters provides a strong foundation for the optimal acquisition and interpretation of the data. Here we present a technical overview of the physics of XCT, describe the major components of a typical laboratory-based XCT instrument, and provide a guide for how to optimize data collection for planetary materials using such systems. We also discuss data processing, visualization and analysis, including a discussion of common data artifacts and how to minimize them. We review a variety of recent studies in which XCT has been used to study extraterrestrial materials and/or to address fundamental problems in planetary science. We conclude with a short discussion of anticipated future directions of XCT technology and application.     

高分辨率光学遥感卫星宽幅成像技术发展浅析

幅宽是影响高分辨率光学遥感卫星应用的重要指标。本文分析了国际上高分辨率光学遥感卫星宽幅成像的主要途径,介绍了多CCD内视场拼接、多相机外视场拼接、敏捷成像、多星组网等主流宽幅成像方式及其数据处理的技术特点,同时分析了相机垂轨摆扫成像、大面阵相机敏捷拼幅成像等新型星载宽幅影像获取方式,有助于系统地了解高分辨率光学遥感卫星宽幅成像技术进展,对于展望其发展趋势具有一定的参考作用。     

分水岭算法在电成像测井图砾石识别中的最优参数研究

基于电成像测井,将分水岭算法应用到电成像测井图砾石的识别中,分水岭算法在砾石识别应用中的参数选取直接影响到识别效果。针对分水岭算法识别砾石的各个步骤,选取不同的优化参数进行处理,对处理效果进行对比分析,最终确定分水岭算法识别砾石的最优参数,并对吉林王府断陷AA井、BB井和CC井三口井进行实际处理,得到很好的效果。     

一种提高储层裂缝识别准确度的方法

油田勘探开发中,储层裂缝的高效、准确识别一直是一个难题。常规测井裂缝识别方法方便但准确度低,电成像测井裂缝识别方法纵向分辨率高、识别准确但人工识别繁琐。为了解决常规和电成像测井裂缝识别方法各自缺点带来的问题,本文提出了一种既高效又准确的储层有效裂缝识别方法。该方法以裂缝在电成像测井上的响应特征为依据,选取裂缝层段为样本,构建常规测井裂缝综合识别因子Y₁和电成像测井裂缝识别因子Y₂,将两因子结合构建储层裂缝识别因子Y₃。利用Y₃识别裂缝,采样点间隔为0.002 54 m,远小于常规测井的0.125 m,比常规测井识别裂缝准确度高;自动拾取裂缝效率远高于繁琐的人工识别,比电成像测井识别裂缝省时省力。将该方法应用到王府地区火山岩储层裂缝识别中可快速准确地识别储层裂缝,准确率达到80%左右,对其他类型储层裂缝研究有一定的借鉴意义。     

临近边坡的条形基础地基极限承载力数值分析

建筑物或构筑物基础临近边坡置放的情况在实际工程中十分普遍,但目前对于临近边坡基础的地基承载力及破坏模式尚缺乏深入研究。采用不连续布局优化（DLO）极限分析法建立数值模型,分析边坡几何尺寸、土体参数和基础位置对临坡条形基础的极限承载力和边坡破坏模式的影响,并对国内外现行规范推荐的计算方法进行评价。结果表明：极限承载力随边坡高度和边坡倾斜角的增大而减小,当坡高超过临界高度后,极限承载力将不受其影响;极限承载力随土体黏聚力和内摩擦角的增大而提高,滑动面随黏聚力的增大而变浅,随内摩擦角的增大而变深;极限承载力随基础与坡肩相对距离的增大而提高,当基础置放位置超过某临界距离后极限承载力不受边坡影响。在土体强度高、坡角较大时,《建筑地基基础设计规范》规定的临坡基础最小置放距离偏于危险,设计时仍需考虑边坡对承载力的减损作用;在土体强度较低、坡角较小时,规范规定值偏于保守。美国AASHTO规范对边坡地基极限承载力的取值在砂土边坡时较为可靠,但其仅适用于坡面破坏模式的情况;饱和黏土边坡的承载力曲线有悖于理论解,对临界距离的规定同样存在低估。     

Cometary cryo-volcanism: Source regions and a model for the UT 2005 June 14 and other mini-outbursts on Comet 9P/Tempel 1

Data on the UT 2005 June 14 mini-outburst of Comet 9P/Tempel 1 taken from different viewpoints have been examined for morphological differences and parallax. The data were taken with the Hubble Space Telescope (HST), from the Deep Impact (DI) spacecraft, and from the Calar Alto Observatory, Spain. The mini-outburst source region was found to be located near 218 ± 6E, 6 ± 5N on the Deep Impact nucleus shape model. The mini-outburst occurred at ∼12 pm local solar time. The distribution of light in the mini-outburst is similar to that expected for an ejecta curtain. The method and software used to determine the surface location was checked using position angles of the impact ejecta plume as seen from DI and HST. The general region of impact was recovered and a downrange tilt of the ejecta curtain axis of 10.2 deg from the surface normal was found. We computed tracks of possible source regions for nine other mini-outbursts seen from DI. Five of these tracks converge on the 2005 June 14 event location. Three of the tracks converge at a second location near (60E, 20S), well separated from the first. Multiple mini-outbursts arise at each location either from a single source or from a few sources in close proximity. The mini-outbursts occur both at night and during the day indicating at most weak, if any, control by direct sunlight. The times of outburst are non-random with a preference for early afternoon, dusk and midnight. None of the mini-outbursts occurred near dawn. They occur at low latitudes (between ±40 deg) near the points where the principal axis of minimum moment of inertia cuts the surface. These regions are furthest from the center of figure and have the lowest effective surface gravity. We use these results to develop a conceptual model of the mini-outburst process and make comparisons with the theoretical calculations. We find that the tensile strength of the sub-surface material must be very low (e.g., ) and, on the basis of features imaged on the western facet of the nucleus, suggest that inflation of the sub-surface may be occurring. Our model makes specific predictions about the kind of surface morphology that should result from mini-outburst activity. We show that one of the isolated rimless depressions and the close-packed depressions found in the Deep Impact images have the properties needed and identify them as possible sites of past and current mini-outburst activity.     

基于超声波合成孔径技术的钻孔成像方法

随着地下空间开发的深入,钻孔岩壁上特殊区域的重视程度越来越高,为了克服传统超声波钻孔成像技术分辨率低的不足,提出一种基于超声波合成孔径技术的钻孔成像方法,提高钻孔图像的分辨率和图像质量。采用高分辨率的合成孔径SAFT成像技术综合处理大量的断面扫描回波信号,达到增强反射信号和抑制干扰信号的目的,使对应的岩壁特征区域回波更加突显,在该基础上提取出扫描断面回波信号的声幅和声时参数。综合声幅和声速参数的特征,提出了基于相关性的超声波钻孔图像重建原则,选择合适的成像数据点,在叠加不同深度的探测数据后形成了关注区域更加明显的钻孔重建图像。将该方法应用到了实际工程中,验证了该方法的可行性和准确性。