一种三维空间9-交模型的简化方法

9-交模型是一种表达三维空间拓扑关系的常用方法,但存在着冗余度大等问题。本文在Z latanova简化9-交模型工作的基础上,定义了点、线、面和体等简单三维空间对象,对它们之间的拓扑关系进行了研究。排除各种不可能的情况,共总结出24种可能的9-交结果以及80种点线面体之间的拓扑关系,并进行归类得到55种拓扑分析操作,从而大大简化了原模型。以线与体的拓扑关系分析为例,给出了根据简化以后的9-交模型进行拓扑分析操作的具体算法实现。     

基于Kinect三维重建的地下井室可视化方法研究

针对现有地下井室病害探测与维护方法的不足,提出了一种基于Kinect三维重建的地下井室可视化方法,以实现其三维可视化探测与维护.还提出了一种基于多项式曲面拟合的Kinect深度测量误差修正方法,利用联合双边滤波算法对深度图像数据进行预处理;结合SIFT特征匹配和改进的RANSAC算法获取相邻点云间的初始位姿,并利用基于...     

基于CATIA三维数模的复合材料复杂曲面展开

采用高斯曲率评估曲面的可展程度,基于复合材料构件的CATIA三维数模,提取三维数模中的铺层信息,生成曲面展开所需要的单层曲面,在CATIA复合材料模块下对铺层曲面进行产品性能分析,确定曲面的不可展性,通过CATIA的"分析与仿真"功能中的高级网格划分模块对单层曲面进行有限元分析,计算出三角网格曲面模型上各点的离散高斯曲率,根据离散高斯曲面曲率最大值所在点,生成将曲面分开的剪口路径,最终将曲面进行展开.     

三元流闭式叶轮组合电加工技术研究Ⅱ——数控电解预加工

数控电解预加工是组合电加工技术中不可或缺的关键工艺,本文专题论述了三元流闭式叶轮数控电解预加工中阴极及其运动轨迹设计等关键技术。提出了采用多个阴极分区域加工流道的方法,利用先层切再叠加的方法将三维问题简化为二维问题处理而实现阴极加工型面的数值求解。在完成阴极结构优化设计专用工装夹具设计和数控加工程序编制的基础上,以某型三元流闭式叶轮为研究对象进行了加工工艺试验,并加工了符合设计要求的三元流闭式叶轮。试验研究表明,采取数控电解预加工工艺方案能够满足实际生产要求,可提高效率40%,降低电火花加工的电极损耗50%。     

γ-ray spectroscopy in Mars orbit during solar proton events

Understanding the evolution of Mars requires determining the composition of the surface and atmosphere of the planet. The European Space Agency’s ExoMars rover mission, which is expected to launch in 2016, is part of the Aurora programme. The instruments on the rover will search for evidence of life on Mars and will map a sub-section of the Martian surface, extracting compositional information. Currently our understanding of the bulk composition (and mineralogy) of Mars relies on orbital data from instruments on-board satellites such as 2001 Mars Odyssey, Mars Reconnaissance Orbiter and Mars Express, in addition to in-situ instrumentation on rovers such as Spirit and Opportunity. γ-ray spectroscopy can be used to determine the composition of Mars, but it has yet to be successfully carried out in-situ on Mars. This study describes some of the results obtained from the γ-ray spectrometer on 2001 Mars Odyssey during solar proton events and discusses whether the increased emissions are useful in γ-ray spectroscopy. The study shows that although increased γ-ray emissions were expected from the Martian surface during a solar proton event, they were not detected from orbit probably due to insufficient signal-to-background. However, this does not preclude the possibility of measuring changes in γ-ray flux corresponding to changes in solar activity on the surface of the planet.     

视觉辅助遥操作在卫星在轨自维护中的应用

为了克服时延对空间机器人遥操作的影响,提出了利用视觉技术辅助遥操作进行卫星自维护的方法.针对遥操作数据传输滞后的问题,设计并实现了一种基于视觉的共享控制策略,该策略将维护任务分为自由空间控制与自主视觉伺服控制.在自由空间控制阶段,通过3D图形预测仿真以及实时反馈的视频流,提高了遥操作者的视觉临场感.在自主控制阶段,采用冗余特征视觉伺服控制,克服了系统对标定精度的依赖性,从而提高了整个系统的智能化程度.最后,通过对典型的卫星维护任务实例的分析,验证了该方法的有效性.     

数字近景摄影大尺寸三坐标测量系统V-STARS的测试与应用

介绍了数字近景摄影大尺寸柔性三坐标测量系统V—STARS的配置、测量原理和测量过程,对其三维坐标及平面度的测量重复性进行了实际测试,与激光跟踪仪进行了平面度的比对测试,并将V—STARS系统成功应用于某17m网状天线的型面测量与调整工程实践中。     

An inversion approach for lunar regolith layer thickness using optical albedo data and microwave emission simulation

An approach to inversion of the lunar regolith layer thickness by using multi-channel brightness temperature observation in passive microwave remote sensing is developed. To first make simulation of brightness temperature from the lunar layered media, the lunar regolith layer thickness (d) is proposed being constructed by available lunar DEM (digital elevation mapping) and on site measurements. The physical temperature distribution (T) over the lunar surface is also empirically assumed as a monotonic function of the latitude. Optical albedo of the lunar nearside from the telescopic observation is employed to construct the spatial distribution of the FeO+TiO₂ content (S) in the lunar regolith layer. A statistic relationship between the DEM and S of the lunar nearside is further extended to construction of S of the lunar farside. Thus, the dielectric permittivity (ε) of global lunar regolith layer can then be determined. Based on all these conditions (d,T,ε), brightness temperature of the lunar regolith layer in passive microwave remote sensing, which is planned for China's Chang-E lunar project, is numerically simulated by a parallel layering model using the strong fluctuation theory of random media.Then, taking these simulations with random noise as observations, an inversion method of the lunar regolith layer thickness is developed by using three- or two-channels brightness temperatures. When the S is low, and the four channels brightness temperatures in China's Chang-E project are well distinguishable, the regolith layer thickness and physical temperature of the underlying lunar rock media can be inverted by the three-channels approach. When the S becomes high that the brightness temperature at high frequency channels such as 19.35, 37 GHz are saturated, the regolith layer thickness is alternatively inverted only by the two-channels approach.Numerical simulation and inversion approach in this paper make an evaluation of the performance for lunar passive microwave remote sensing, and for future data calibration and validation.     

Nb-10Si合金室温断裂韧性研究

利用真空电弧熔炼制备了处于亚共晶区的Nb-10Si-xMo(x=5,15)复合材料,采用扫描电子显微镜(SEM)和X射线衍射(XRD)分析了在1200℃退火100h后复合材料的微观组织形貌、相组成和断口形貌,并测定了Nb-10Si-Mo复合材料的显微硬度。用单边切口悬臂梁法(SENB)研究了加入合金元素后复合材料室温韧性的变化。深入分析了合金元素对材料韧性相变形行为和复合材料室温断裂韧性的影响。     

某小型涡扇发动机全流道准三维数值法

采用高阶精度Godunov格式和时间相关法,用多部件模型在小型涡扇发动机的全流道S2流面上求解带黏性力项的非定常Euler方程组,并将整机模拟的结果与试验结果进行了对比,在合理给出损失的情况下,计算结果与试验结果基本吻合.