对空间碎片的相对位姿估计

针对几何、质量特性参数均未知的空间碎片,提出一种基于扩展卡尔曼滤波（EKF）的相对位姿估计算法。该算法以单目相机获得的目标图像特征视线信息作为测量输入,以目标姿态、姿态角速度、惯量比、相对位置、相对速度和特征位置作为滤波状态。对算法进行可观性分析,给出两个可以保证算法可观性的条件。分别针对不同条件进行数值仿真,仿真结果表明新算法能够对几何和质量参数未知的空间碎片进行有效的相对位姿 估计。     

Milling surface roughness for 7050 aluminum alloy cavity influenced by nozzle position of nanofluid minimum quantity lubrication

In nanofluid minimum quantity lubrication (NMQL) milling of aviation aluminum alloy, it is the bottleneck problem to adjust the position parameters (target distance, incidence angle, and elevation angle) of the nozzle to improve the surface roughness of milling, which has large and uncontrollable errors. In this paper, the influence law of milling cutter speed, helical angle, and cavity shape on the flow field around the milling cutter was studied, and the optimal nozzle profile parameters were obtained. Using 7050 aluminum alloy as the workpiece material, the milling experiment of the NMQL cavity was conducted by utilizing cottonseed oil-based Al₂O₃ nanofluid. Results show that the high velocity of the surrounding air flow field and the strong gas barrier could be attributed to high rotating velocities of the milling cutter. The incidence angle of the nozzle was consistent with the helical angle of the milling cutter, the target distance was appropriate at 25–30 mm, and the elevation angle was suitable at 60°–65°. The range and variance analyses of the signal-to-noise ratio of milling force and roughness were performed, and the chip morphology was observed and analyzed. The results show that the optimal combination of nozzle position parameters was the target distance of 30 mm, the incidence angle of 35°, and the elevation angle of 60°. Among these parameters, target distance had the largest impact on cutting performance with a contribution rate of more than 55%, followed by incidence angle and elevation contribution rate. Analysis by orthogonal experiment revealed that the nozzle position parameters were appropriate, and R_a (0.087 μm) was reduced by 30.4% from the maximum value (0.125 μm). Moreover, R_sm (0.05 mm) was minimum, which was 36% lower than that of the seventh group (R_sm = 0.078 mm).     

基于正态云模型的方法求解目标可能位置域

面向辅助决策军事需求的原则,介绍了定性与定量之间的不确定性转换模型-正态云模型。综合该模型的模糊性和随机性,求解导弹攻击敌方水面舰艇的可能位置域。     

光纤陀螺/GPS组合导航系统中的信息融合技术

光纤陀螺捷联惯导系统用于导航定位具有自主性的优点,但系统误差随时间累积.全球定位系统(GPS,Global Position System)用于导航定位精度很高,误差不随时间积累,但抗干扰性能很差,没有自主性.运用信息融合技术将光纤陀螺捷联系统和GPS进行组合,将GPS的高度信息引入惯导高度反馈通道,设定反馈系数,抑制高度发散,将GPS经度、纬度、地速信息作为系统卡尔曼滤波器量测信息,消除惯导积累误差.提出的信息融合方案运用于某中精度光纤陀螺/GPS组合导航系统并进行路试,导航系统输出3个方向位置数据与定位基准相比,误差不随时间积累,路试结果表明此信息融合方案的有效性及工程的实用性.      

基于特征光点单坐标系坐标的运动目标相对位置姿态光学测量方法

针对运动目标的相对位置姿态测量问题,研究了一种利用四个非共线特征光点的光学 测量方法。推导了基于特征光点目标坐标系和测量坐标系坐标的运动目标相对位置姿态解算 公式;进而给出了基于特征光点单坐标系坐标的位置姿态的解析解;并建立了测量的误差模 型。该方法对特征光点布局要求低,对摄像机模型没有限制。实验结果表明,该方法可满足 运动目标的相对位置姿态测量需求。     

相敏检波法在硬支承动平衡检测中的应用

为了检测硬支承情况下转子的不平衡量,针对目前常用相敏检波电路的缺点,提出了一种模拟乘法器式检测转子旋转过程中不平衡量大小和相位的相敏检波法。描述了此方法的原理,运用此方法设计了检测电路,实现了预期的目的。     

经济型轴类零件形位误差测量仪的研制

在偏摆仪基础上,以ＭＣＳ－５１单片机为核心,研制了“经济型轴类零件形位误差测量仪”。介绍了测量仪的机械结构、硬件电路及软件设计原理,并对测量仪的误差进行了分析。该仪器可用于圆度、轴线直线度、同轴度和径向跳动误差等项目的测量。     

基于计算博弈的脉冲作用下航天器追逃策略

本文研究了地球高阶引力模型中,基于脉冲作用的航天器轨道追逃问题。针对该问题,将航天器轨道追逃问题定义为两选手计算博弈,其中以博弈双方的距离和燃料消耗设计了性能指标函数,并以速度增量大小和方向构建容许控制集。此外,为了保证纳什均衡解的求解效率,引入了快速搜索(ARS)算法,并设计了一种数据剪枝方法用于优化搜索空间,最终实现了基于计算博弈的控制策略的快速求解。仿真结果表明:该方法能够有效解决脉冲作用下航天器的追逃难题,与传统方法相比,该方法能同时满足脱靶量精度和燃料消耗要求,具有一定的可行性和有效性。     

1996-2003年大耀斑事件引起的TEC突然增强的统计分析

利用1996—2003年期间GOES卫星耀斑观测资料和国际GPS观测网的GPS—TEC资料分析X级大耀斑事件引起的电离层电子浓度总含量(TEC)的突然增强(SITEC)现象．对X射线耀斑等级、耀斑日面位置与SITEC的关系进行了分析．结果表明,两者都与SITEC现象的强弱有着一定的正相关性．在消除X射线耀斑等级、耀斑日面位置对电离层SITEC现象的影响后,进而分析了日地距离以及耀斑持续时间对电离层SITEC现象的影响．结果表明,日地距离和耀斑持续时间都是影响SITEC现象的重要参数,日地距离较近时发生的耀斑事件引起的SITEC现象较为强烈．另外,耀斑持续时间越长,SITEC现象越微弱,但是当耀斑持续时间继续延长时,SITEC现象的强弱逐渐趋于不再改变,最后在某值附近达到平衡．还对某些没有在电离层中引起明显SITEC现象的耀斑事件进行了讨论,发现了这类耀斑的一些特征．     

Artificial equilibrium points and bi-impulsive maneuvers to observe 243 Ida

In the restricted three-body problem, the traditional Lagrange points L₁ and L₂ are the only equilibrium points near the asteroid 243 Ida. The thrust generated by a solar sail over a spacecraft enables the existence of new artificial equilibrium points, which depend on the position of the spacecraft with respect to the asteroid and the attitude of the solar sail. Such equilibrium points generate new spots to observe the body from above or below the plane of motion. Such points are very good observational locations due to their stationary condition. This work provides a preliminary analysis to observe Ida through the use of artificial equilibrium points as spots combined with transfer maneuvers between them. Such combination can be used to observe the asteroid from more different points of view in comparison to fixed ones. The analyses are made for a spacecraft equipped with a solar sail and capable of performing bi-impulsive maneuvers. The solar radiation pressure is used both to maintain the equilibrium condition and to reduce the costs of the transfers and/or to create transfers with longer duration. This is a new aspect of the present research, because it combines the continuous thrust with initial and final small impulses, which are feasible for most of the spacecraft, because the magnitudes of the impulses are very low. These combined maneuvers may reduce the transfer times of the maneuvers in most of the cases, compared with the maneuvers based only on continuous thrust. Several options involved in these transfers are shown, like to minimize the fuel spent ($\mathrm{\Delta }\mathit{v}$) as a function of the transfer time or to extend the duration of the travel between the points. Extended transfer times can be useful when observations are required during the transfers.