基于相位匹配的大视场视觉检测系统

针对三维测量大量程和高精度测量问题,提出一种新型双目视觉检测系统.该系统通过向被测物投射间距可变的光栅条纹,将不同曲率的被测表面进行相位编码,由相位匹配得到被测物稠密的立体匹配点云;再由标定出的摄像机内外参数计算出被测物的精确三维坐标.为了解决传感器单元测量区域较小的问题,系统通过步进电机控制传感器移动,获取大型物体的全场三维数据点云;最后利用四元素法,实现大型物体的三维数据拼接.该系统长度测量标准差为36 μm,角度测量与坐标测量机(CMM)测量结果的相对误差0.2％.给出了某V型面三维实测的数据重建结果.对某大型特件(360 mm×300 mm)经过三维拼接正确复现了其三维形貌.该系统对于解决大型构件三维形貌的在线高精度检测问题具有较高工程应用价值.      

星载SAR相控阵天线热变形误差分析

根据星载SAR相控阵天线结构特点,建立了天线热变形误差的数学模型,定义了阵面不平整度指标.基于成对回波畸变理论,推导了天线阵面存在热变形误差时的方向图函数表达式,导出了单频热变形误差分量与模糊度之间的统计关系,提出了定量分析星载SAR相控阵天线热变形误差对模糊性能影响的有效方法.基于L波段星载SAR天线进行了计算机仿真,验证了分析方法的正确性.      

金属/水反应冲压发动机三维内流场数值模拟

采用颗粒轨道模型进行了燃气发生器式金属/水反应冲压发动机补燃室两相流的数值模拟,建立了水冲压发动机补燃室反应流模型,并对某发动机进行了模拟,研究了一次进水时不同喷注位置和喷孔个数对铝颗粒燃烧效率和发动机性能的影响规律,得出了反应物和产物组分、温度等发动机参数的变化趋势。结果表明,存在使发动机性能达到较优的进水位置,一次进水以2孔对称分布为宜。模拟结果可为发动机设计提供参考。     

基于空间交会的天基反卫作战方案

对位于高地球轨道天基平台攻击低地球轨道目标的方案进行了研究,讨论了高轨作战平台的攻击范围。采用完全推力法实现远程空间交会。为消除异面霍曼变轨方法等待时间过长的缺点,提出了两种主动调相方法。研究表明：用该法可实现天基武器由高轨至低轨的空间转移交会,引入主动调相轨道可明显缩短交会所需时间。     

考虑地球非球形摄动的固体动能拦截器助推段最优控制方案研究

针对三维空间内的高速飞行目标,提出了一种可用于固体动能拦截器助推段的精确最优控制方法。考虑了地球非球形摄动的影响,建立了有限推力拦截器最优控制问题动力学模型,并用直接配置法与SQP方法进行了数值求解,得到了更加精确的助推段控制方案。算例证明该方法有效。     

频率合成器相位噪声对跳频通信系统的影响

宽带、高速跳频频率合成器是整个跳频通信系统的核心,其输出信号的相位噪声对系统性能的影响不可忽略。它将限制接收机能得到的最大信噪比,导致接收机灵敏度下降,同时降低数字解调器的性能。文章首先从理论上分析了相位噪声对跳频通信系统的影响,然后结合实际的数传系统,对相噪进行了仿真,仿真结果证明了理论分析的正确性。     

基于单频GPS的单点测浪方法的研究

介绍一种用单频单台GPS接收机解算其相对位置变化的算法—PVD算法的基本原理,针对它在海浪测量应用中的特点,提出基于海浪谱估计的自适应PVD算法。实测数据的处理结果表明,用自适应PVD算法解算出的浪高可达厘米级精度。     

浅论飞机维修生产计划与控制优化

探讨了通过优化维修生产和控制环节,即优化从维修方案到组包控制方式的流程,实现获得最小的飞机停场时间(最大可用率)、资源的最大化利用和最小的维修成本。     

Integer phase ambiguity estimation in next-generation geodetic Very Long Baseline Interferometry

Next-generation Very Long Baseline Interferometry (VLBI) system designs are aiming at 1 mm global position accuracy. In order to achieve this, it is not only necessary to deploy improved VLBI systems, but also to develop analysis strategies that take full advantage of the observations taken. Since the new systems are expected to incorporate four independent radio frequency bands, it should be feasible to resolve phase ambiguities directly from post-correlation data, providing roughly an order of magnitude improvement in precision of the delay observable. As the unknown ambiguities are of integer nature, it is discussed here how they the can be resolved analytically using algorithms which have been developed for Global Navigation Satellite System (GNSS) applications. Furthermore, it will be shown that ionosphere contribution and source structure effects, so-called core-shifts, can be solved simultaneously with the delay, which is the main geodetic observable for follow-on analysis. In order to verify the proposed algorithm, simulated observations were created using parameters from actual design studies. It is shown that, even in the case of low signal-to-noise ratio observations, reliable phase ambiguity resolution can be achieved and it is discussed how the integer ambiguity recovery depends on the number of observations and signal-to-noise ratio.     

Relationship of the diffuse aurora and SAR arc dynamics to substorms and storms

Investigation results of a diffuse aurora (DA) and stable auroral red (SAR) arc dynamics based on spectrophotometric observations at the Yakutsk meridian (199°E geomagnetic longitude) are presented. The relationship of an equatorward extension of DA in the 557.7 nm emission to a substorm growth phase during the magnetospheric convection intensification after the turn of IMF B_Z to the south is shown. The formation of SAR arc during the substorm expansion phase is investigated. The association of SAR arc dynamics with the development of asymmetric ring current (substorm injection) during the main phase of a storm is analyzed. It is shown how the pulsating precipitations of energetic ring current particles develop in the outer plasmasphere based on photometric observations.