多轴联动条件下插补速度实时可调的前瞻控制算法

针对目前多轴联动条件下S形加减速算法复杂,一条插补线段内最大进给速度不能实时可调的问题,提出了一种插补速度实时可调的前瞻控制算法。算法首先根据机床特性和线段夹角建立了小线段衔接处进给速度的约束条件,然后采用加速度跟随原理提出了最大进给速度连续可调的S形加减速控制方法,在此基础上设计了一种加速度自适应调整的前瞻处理算法。该算法在不降低轨迹插补精度的前提下,能以最大的速度通过线段的转接点,从而使整个线段插补过程具有高度的柔性和快速性,能满足现代数控系统对前瞻处理的实时性要求。结果表明该算法有效降低了机床运动时的振动,与传统速度规划算法相比,同等加工条件下,加工效率明显提高,工件表面质量也得到改善。     

挠性航天器姿态机动的变论域自整定模糊PID控制

建立了带有太阳翼的挠性航天器的姿态动力学模型,应用改进的罗德里格参数来描述姿态运动学模型。针对挠性航天器模型参数不确定性和环境干扰等问题,提出了变论域自整定模糊比例积分微分(PID)控制方案,构建了计算简单并且可以达到控制精度的伸缩因子。基于Matlab/Simulink进行了仿真验证,结果表明,变论域自整定模糊PID 控制响应速度比传统PID控制、模糊PID控制快350s,且无超调,不仅能够使航天器完成对目标姿态的机动,而且能够有效地抑制挠性太阳翼的振动。     

中继卫星S/Ka双频地面站天线共用跟踪接收机

论述了Ka频段圆波导TE11和TE21模自跟踪体制和S频段正十字排列四喇叭自跟踪体制共用两信道自跟踪接收机问题.导出了来波及地面天线S频段和、差信道极化特性引起的角误差电压的交叉耦合系数公式.还可以进一步使S/Ka两个频段共用一套能跟踪（直接序列）扩频信号源的伪单脉冲（单信道单脉冲）自跟踪接收机.     

锂氟化碳电池对火星探测任务工况适应性研究

锂氟化碳电池在固体正极体系一次电池中拥有最高的理论比能量(约2180 W·h·kg-1),特别适合对载荷质量要求苛刻的深空探测任务.我国首个火星探测器"天问一号"在其着陆巡视器内部使用了一组锂氟化碳电池用于完成进入—下降—着陆段的供电任务.文章提炼锂氟化碳电池与深空探测应用密切相关的4项基本特性,根据火星探测任务的特点...     

基于IFS和IPSO算法的干扰资源分配方法

针对多干扰系统同时干扰多部雷达的干扰资源分配问题,提出一种基于直觉模糊集(IFS)和改进粒子群优化(IPSO)算法相结合的干扰资源分配方法。利用己方无源探测系统获得的敌方雷达参数,根据IFS理论得到敌方雷达的威胁系数;整合数据库中战场的己方干扰系统与敌方雷达系统信息,从空域、频域、极化方式和干扰样式4个方面定义了匹配度,表示己方干扰系统对敌方雷达系统的干扰效率,得到匹配度矩阵,结合敌方雷达威胁系数建立干扰目标函数;提出一种自适应调整权重、异步变化学习因子、针对离散问题的IPSO算法,并引入补偿粒子进行盲区搜索,求解出最佳干扰决策。仿真表明,本文提出的干扰资源分配方法相较于传统算法最优解正确率更高,且实时性更好。     

Fault diagnosis of an intelligent hydraulic pump based on a nonlinear unknown input observer

Hydraulic piston pumps are commonly used in aircraft. In order to improve the viability of aircraft and energy efficiency, intelligent variable pressure pump systems have been used in aircraft hydraulic systems more and more widely. Efficient fault diagnosis plays an important role in improving the reliability and performance of hydraulic systems. In this paper, a fault diagnosis method of an intelligent hydraulic pump system (IHPS) based on a nonlinear unknown input observer (NUIO) is proposed. Different from factors of a full-order Luenberger-type unknown input observer, nonlinear factors of the IHPS are considered in the NUIO. Firstly, a new type of intelligent pump is presented, the mathematical model of which is established to describe the IHPS. Taking into account the real-time requirements of the IHPS and the special structure of the pump, the mechanism of the intelligent pump and failure modes are analyzed and two typical failure modes are obtained. Furthermore, a NUIO of the IHPS is performed based on the output pressure and swashplate angle signals. With the residual error signals produced by the NUIO, online intelligent pump failure occurring in real-time can be detected. Lastly, through analysis and simulation, it is confirmed that this diagnostic method could accurately diagnose and isolate those typical failure modes of the nonlinear IHPS. The method proposed in this paper is of great significance in improving the reliability of the IHPS.     

Super-resolution reconstruction of astronomical images using time-scale adaptive normalized convolution

In this work, we describe a new multiframe Super-Resolution (SR) framework based on time-scale adaptive Normalized Convolution (NC), and apply it to astronomical images. The method mainly uses the conceptual basis of NC where each neighborhood of a signal is expressed in terms of the corresponding subspace expanded by the chosen polynomial basis function. Instead of the conventional NC, the introduced spatially adaptive filtering kernel is utilized as the applicability function of shape-adaptive NC, which fits the local image structure information including shape and orientation. This makes it possible to obtain image patches with the same modality, which are collected for polynomial expansion to maximize the signal-to-noise ratio and suppress aliasing artifacts across lines and edges. The robust signal certainty takes the confidence value at each point into account before a local polynomial expansion to minimize the influence of outliers. Finally, the temporal scale applicability is considered to omit accurate motion estimation since it is easy to result in annoying registration errors in real astronomical applications. Excellent SR reconstruction capability of the time-scale adaptive NC is demonstrated through fundamental experiments on both synthetic images and real astronomical images when compared with other SR reconstruction methods.     

运动声呐空时自适应处理中的多普勒影响分析

为了将空时自适应处理(STAP)理论更好地应用于水下环境,提高运动声呐对混响的抑制性能,研究了多普勒对运动声呐STAP的影响。具体分析了由多普勒造成的回波脉宽伸缩变换以及目标空时导向向量失配带来的影响。分析结果表明,回波包络脉宽变化对于匹配滤波输出信噪比影响较小,而对空时导向向量修正可以有效提高目标方位估计精度以及混响抑制能力。     

光纤陀螺本征频率对准误差引起的零偏漂移抑制方法

在温度环境下,光纤环的伸缩及光折射率的变化等会引起光纤陀螺本征频率发生变化,产生光纤陀螺本征频率与陀螺调制频率对准误差,进而导致探测器信号中的“尖峰脉冲”信号发生变化,使光纤陀螺产生零偏漂移。通过分析光纤陀螺本征频率的变化,提出了一种调制频率自动跟踪本征频率的方法,从而减小了温度条件下光纤陀螺的零偏漂移。试验验证结果表明,采用该方法的光纤陀螺在-40℃～+60℃的温度范围内固定温度点下的零偏极差减小了50%。     

基于结构张量特征的机体损伤区域动态划分

为提升飞机结构损伤维修分析的智能化水平,实现飞机结构损伤模型的高效重构,提出了基于结构张量特征的动态阈值损伤区域划分方法。首先,引入结构张量理论,特征表示图像局部颜色结构纹理,完备损伤图像特征表示;其次,通过构建共性分布的结构张量特征空间,从而使不同损伤图像具有一致性损伤区域划分流程;在此基础上,定义了动态阈值划分算子,并通过对动态阈值划分算子参数的计算,实现结构张量特征空间中的动态阈值划分;最后,选用不同飞机结构损伤实例图像对方法进行了对比验证。验证结果表明,相比于传统灰度方法、固定阈值划分和其他动态阈值划分算子,椭圆算子划分得到的损伤边界连贯完整,能够有效分割微小裂纹,噪点较少,质量较优。该方法运算高效、流程统一、特征表示完备,对不同类型结构损伤的适用性好。