基于三维激光扫描技术的岩质边坡泥化夹层空间分布和几何形态

为了定量研究泥化夹层的空间分布和几何形态,以云南省玉溪市生活垃圾焚烧发电厂高边坡局部开挖剖面为对象,利用徕卡ScanStation C10三维激光扫描仪和瑞典ROMER RA-7520-2六轴关节臂三维测量仪进行扫描,得到了开挖剖面和泥化夹层的原始点云数据;然后采用Cyclone和Geomagic Wrap软件对点云数据进行一系列处理,分析了泥化夹层的三维空间分布、层面产状、间距、层面粗糙度和几何形态。结果表明：大部分泥化夹层横向分布于整个扫描剖面,少数呈局部分布;泥化夹层的平均倾向为196.41°±5.51°,平均倾角为22.27°±2.23°,间距在3.7~49.1 cm之间,平均值为（20.4±12.0）cm;不同层位及同一层位不同横向位置的泥化夹层厚度都不等,最厚约20 mm,最薄小于1 mm;泥化夹层顶面局部典型区域的平面拟合偏差在-22.4~32.5 mm之间,沿夹层倾向的粗糙度系数在5.67~16.77之间,平均值为10.11±3.25;泥化夹层的表面积与体积之比在5.14~5.86 cm^-1之间。运用三维激光扫描技术研究泥化夹层的空间分布和几何形态是可行的。玉溪市生活垃圾焚烧发电厂高边坡的泥化夹层具有宏观整体上相对平直、相互近似平行、非等距分布、间距小、层数多、厚度薄,细观上顶面粗糙底面相对光滑、三维形态复杂的特点。     

Effects of long-term cyclic horizontal loading on bucket foundations in saturated loose sand

A 1-g model experimental study was conducted to investigate the accumulated rotations and unloading stiffness of bucket foundations in saturated loose sand. One-way horizontal cyclic loading was applied to model bucket foundations with embedment ratios 0.5 and 1.0. Up to 10⁴ cycles of loading were applied at a frequency of 0.2 Hz varying load amplitudes. The accumulated rotation of the bucket foundations increased with the number of cycles and the load amplitudes. Empirical equations were proposed to describe the accumulated rotation of the foundations. The unloading stiffness of foundations increased with the number of cycles but decreased with an increase in load amplitude. The initial unloading stiffness of L/D = 1.0 (L is skirt length; D is foundation diameter) was approximately twice that of L/D = 0.5. Excess pore water pressure difference of 50% was observed between L/D = 0.5 and 1.0. The suction and static capacity of the bucket increased with increase of bucket embedment ratio with a difference of 69.5% and 73.6% respectively between L/D = 0.5 and 1.0.     

新型移动三维激光扫描技术在盾构管片椭圆度检测中的应用

铁运营阶段对隧道结构的变形监测保证了地铁运行的安全,而椭圆度检测是地铁隧道结构检测的重要工作。本文简单介绍了传统椭圆度检测的基本方法,分析了新型移动三维激光扫描检测系统基本原理及隧道椭圆度检测的方法和处理流程。通过工程案例实际应用以及对检测结果的综合分析,证明了移动三维激光扫描技术在盾构管片椭圆度检测中的优势。     

基于激光点云的巨型倾倒大变形体监测研究

以某特高岸水库巨型变形体为研究对象,应用地面三维激光扫描仪采集变形体表面激光点云数据,建立变形体DEM模型,几何量测提取点、线、面(体)成果,对比及叠加分析,得到特定点、线、面及整个变形体位移量信息。研究结果表明,高密度激光点云数据可弥补传统监测成果单一及分析局限或以点概全的不足,以其丰富多样的监测成果全面反映变形体的变形信息,尤其对速滑变形在时效性和精度匹配上更有效,可达到应急预报要求。     

耀变体在射电波段的偏振研究

利用UMRAO数据库22个耀变体源的偏振数据,根据Lazarian&Pogosyan理论模型分析研究了耀变体射电波段的偏振随波长的变化,得出不同类的耀变体偏振随波长变化的原因。结果表明,与Lazarian&Pogosyan理论模型吻合较好。由此得出如下结论:(1)反常去偏振耀变体源中反常法拉第旋光起主导作用,反常去偏振相对较少;(2)热辐射与同步辐射混合作用,高频波段的偏振度小于低频波段的偏振度(反常去偏振);(3)当被观测波段波长小于吸积盘热辐射对应的维恩波长时,高频波段的偏振度大于低频波段的偏振度(常规去偏振)。     

南山26米射电望远镜轨道高差测量及其对指向精度的影响

轮轨式天线的轨道作为承载整个天线重量的基础,其精度直接影响天线在方位方向运转的平稳性,引起天线轴系偏差从而影响天线的指向精度。介绍改造后的乌鲁木齐南山26 m射电望远镜(Nanshan Radio Telescope, NSRT)轨道结构以及轨道高差测量,并建立天线在不同方位、俯仰角下轨道高差引起天线指向偏差的数学模型。利用"十字扫描"法实测多颗标准源在相应位置的指向数据,并通过高斯拟合得到指向偏差。通过分析可知,轨道高差引起的指向偏差经过修正可以提高天线的指向精度。     

徕卡RTC360三维激光扫描仪在竣工测量中的应用

徕卡RTC360不仅操作简单、扫描速度快,而且非常智能。可以实时跟踪计算两个连续站点间的相对位置,点云实时预拼接。后期搭配Register360智能拼接软件,点云智能拼接处理,无需人工干预,简单高效。     

运用人工鱼群算法的3D扫描碎片重建探究

针对传统三维碎片拼接匹配过程中依赖单一特征及存在误差累积的问题,提出了一种运用鱼群算法的全局最优匹配方法。该方法先对碎片点云数据进行多特征提取,结合纹理、专家经验信息对混合在一起的多种类型碎片进行粗糙集分类,之后采用鱼群算法的最优解求得最佳匹配方案。实例验证所提全局匹配方法具有能力强、与初始位置无关及较强的稳健性等特点,为三维碎片的全局匹配提供了一种有效的解决方案。     

基于投影变换的线阵旋转扫描相机标定方法

针对线阵旋转扫描相机标定数据难以获取及模型解算不稳定的问题,提出了一种基于投影变换的线阵旋转扫描相机标定方法。首先构建了一种新的线阵旋转扫描相机成像模型,该模型可以根据相机旋转平台参数、线阵旋转扫描相机成像平面与其切平面的位置关系将旋转扫描图像投影为框幅式图像;然后根据构建出的成像模型,采用直接线性变换法和非线性优化方法进行相机标定和参数优化。试验结果表明,此方法简单易行,具有较高的精度。     

The influence of the electromagnetic core-mantle coupling torques on earth's rotation

The electromagnetic core-mantle coupling is one of the most likely hypotheses to explain the connections between both, the decade fluctuations of the Earth rotation and such of the magnetic field of the Earth. Within this paper, the axial and equatorial electromagnetic torques are computed at time intervals of two years from 1903.5 to 1975.5. They are compared with mechanical torques necessary for the excitation of the decade variations of the rotation of the Earth. The comparison is made with regard to the magnitude of the torques, to their time behaviour and to the periods within the time variations of both types of the torques. The computed electromagnetic torques are comparable with that necessary to excite the variations of the rotation of the Earth. But they are two or three orders less than that necessary to excite the decade variations of the polar motion. Some comparable periods were found within the spectra of the electromagnetic and the mechanical torques. This speaks in favour of the core-mantle coupling. But there are differences between both spectra too hinting at other processes which we cannot describe by a simple model of the core-mantle coupling.