基于结构光扫描数据点的内表面重建方法

提出基于结构光扫描获取的特征点重建物体内表面的方法.结构光扫描获取原始数据精度较高,但是存在数据密度不均的问题.通过剔除测量方向部分冗余数据点和插补扫描方向的稀疏数据,对原始三维数据密度进行适当调整,然后采用基于局部切平面簇的方法对调整后的数据点云进行表面重建.在某一特征点的邻域构造对应于该点的局部切平面,通过局部切平面簇逼近原始表面,采用Marching cubes算法提取等值面,得到三维表面重建的初始网格,根据优化算法简化网格,并采用Loop细分法平滑网格,获得描述物体表面特征的重建表面.该方法解决了由结构光扫描获取的不均匀原始数据点重建物体内表面的问题.      

基于N-S方程的尾迹面法翼型气动阻力计算

研究了计算翼型阻力改进的方法——尾迹面法及尾迹面积分的位置和相应的积分技术.在亚跨声速时分别采用了表面积分和尾迹积分求得给定翼型RAE2822的阻力.结果显示,2种方法具有相同的结果,表明尾迹面积分方法是有效的,与实验值吻合较好.尾迹面法中,尾迹面位置应处于离后缘相对弦长距离0.6~1.0之间.尾迹面积分方法中积分结果不依赖于物体的详细几何外形,可以预计对曲率变化大的三维复杂外形,该方法有更大的优势.      

时隙分配算法在CDM GDP 程序中的应用

机场容量由于恶劣天气等突发原因受到限制导致大面积航班的延误,带来了巨大的经济损失.CDM(Collaborative Decision Making) GDP(Ground Delay Procedure)就是解决这类突发情况的空中交通流量管理程序.就其核心问题——时隙分配,在现有的时隙分配算法基础上,引入航班延误损失系数,使得算法以延误损失替代延误时间,提出了2种基于该系数的时隙分配算法.最后,用java语言进行了仿真实验,引入了评判函数来选择在总延误损失和延误损失分配的公平性上最佳满足决策者要求的分配结果.      

CCSDS图像无损压缩标准在恒速信道中的应用研究

在CCSDS建议的无损数据压缩的基本原理上 ,结合基于局域纹理特征的处理方法 ,给出数据输入输出在恒速信道条件下一种有效的面向空间应用的遥感图像无损压缩方案。该方案包括去相关处理、熵编码以及压缩缓存控制三部分。去相关操作是在局域纹理分析方法的基础上 ,通过提取两种有效的预测模型并自适应选择最佳的模型进行处理 ;然后采用快速有效的CCSDS熵编码器对最佳去相关模型的预测误差编码。在压缩方案中充分考虑了输入输出恒速信道条件下应用的特殊性 ,设计了相应的压缩码流控制方法 ,从而给出了一套有效的针对恒速输入输出信道条件下的图像无损压缩的应用方案     

图象压缩技术的发展

图象压缩是信息领域发展中的关键技术之一,本文综述了图象压缩技术的发展,论述了各发展阶段的基本压缩原理、特点及主要实用方法的优缺点。对80年代后期新发展的分数维压缩方法的有关概念、方法及现状着重作了论述。分数维图象压缩方法与VLSI技术的结合,将会对未来的遥感、通讯、导航及一切与图象有关的领域产生重大影响。     

一种新型恒温—温补晶体振荡器

提出了一种ＯＣＸＯ的恒温控制方法。该方法是利用乙醇的沸点制成换态式恒温箱。这种温度控制方法既可以用作中准确度的ＯＣＸＯ，又可以作为精密双层控温ＯＣＸＯ的外层恒温装置，还可以与简单的温补线路结合，构成高准确度的ＯＴＣＸＯ。     

大型航天器SGCMG系统的奇异性分析研究

应用单框架控制力矩陀螺系统（SGCMG）是大型航天器姿控系统较为理想的选择，但是该系统存在严重的奇异现象，增加了操纵律的设计与开发的难度。文章从奇异性分析的角度对单杠架控制力矩陀螺系统的奇异状态进行了研究，提出了奇异可回避性的判别方法，并据此对SGCMG系统奇异状态进行了系统的分类，针对常用的各种构形的SGCMG系统进行了讨论。     

Effects on winter circulation of short and long term solar wind changes

Indices of the North Atlantic Oscillation and the Arctic Oscillation show correlations on the day-to-day timescale with the solar wind speed (SWS). Minima in the indices were found on days of SWS minima during years of high stratospheric aerosol loading. The spatial distribution of surface pressure changes during 1963–2011 with day-to-day changes in SWS shows a pattern resembling the NAO. Such a pattern was noted for year-to-year variations by Boberg and Lundstedt (2002), who compared NAO variations with the geo-effective solar wind electric field (the monthly average SWS multiplied by the average southward component, i.e., negative Bz component, of the interplanetary magnetic field). The spatial distribution of the correlations of geopotential height changes in the troposphere and stratosphere with the SWS; the geo-effective electric field (SWS∗Bz); and the solar 10.7 cm flux suggests that solar wind inputs connected to the troposphere via the global electric circuit, together with solar ultraviolet irradiance acting on the stratosphere, affect regional atmospheric dynamics.     

Dynamics and control of spacecraft hovering using the geomagnetic Lorentz force

To achieve hovering, a spacecraft thrusts continuously to induce an equilibrium state at a desired position. Due to the constraints on the quantity of propellant onboard, long-time hovering around low-Earth orbits (LEO) is hardly achievable using traditional chemical propulsion. The Lorentz force, acting on an electrostatically charged spacecraft as it moves through a planetary magnetic field, provides a new propellantless method for orbital maneuvers. This paper investigates the feasibility of using the induced Lorentz force as an auxiliary means of propulsion for spacecraft hovering. Assuming that the Earth’s magnetic field is a dipole that rotates with the Earth, a dynamical model that characterizes the relative motion of Lorentz spacecraft is derived to analyze the required open-loop control acceleration for hovering. Based on this dynamical model, we first present the hovering configurations that could achieve propellantless hovering and the corresponding required specific charge of a Lorentz spacecraft. For other configurations, optimal open-loop control laws that minimize the control energy consumption are designed. Likewise, the optimal trajectories of required specific charge and control acceleration are both presented. The effect of orbital inclination on the expenditure of control energy is also analyzed. Further, we also develop a closed-loop control approach for propellantless hovering. Numerical results prove the validity of proposed control methods for hovering and show that hovering around low-Earth orbits would be achievable if the required specific charge of a Lorentz spacecraft becomes feasible in the future. Typically, hovering radially several kilometers above a target in LEO requires specific charges on the order of 0.1 C/kg.