一类不确定混沌系统的强鲁棒跟踪控制

基于指数终端吸引子的有限时间快速收敛特性,将指数型快速终端滑模引入一类不确定混沌系统,提出了一种新的滑模变结构跟踪控制。证明了系统跟踪误差变量在有限时间内能以较快的收敛速度到达各级滑模面的邻域,并最终收敛至平衡点附近很小的区域,系统有良好的动态性能。Dulling系统仿真结果表明该控制策略有强鲁棒性。     

Heat Absorbing and Releasing Experiments with Improved Phase-change Thermal Storage Canisters

This article, based on authors' long-term study, proposes an improved foamed-Ni-packed phase-change thermal storage canister, which takes advantage of the foamed-Ni characteristic of instinctive porous structure and excellent properties to ameliorate its void distribution and thermal conductivity. The improved canister and the unimproved one without foamed-Ni package, are put to heat absorbing and releasing tests to investigate the effects of heat absorbing temperature upon the phase-change materials (PCM) melting time under three temperature schemes by using platinum resistance thermometers (PT100) and data acquisition modules (ADAM-4000) to gather the data of varying temperature. Afterwards, the computerized tomography (CT) is employed to scan the void distribution in both canisters. Compared to the unimproved canister, the experimental results evidence the superiority of the improved one in higher uniformity in void and temperature distribution as well as faster thermal responses.     

微波延迟线量值溯源研究

针对微波延迟线量值溯源的问题,提出了有效的量值溯源方法。简析了微波延迟线的结构及技术参数,阐述了微波传输电缆和声体波两种延迟线延迟时间的测量方法,分析并提出了用通用计量器具和专用计量器具对延迟时间进行量值溯源的两种方法。     

基于杂波子空间估计的MIMO雷达降维STAP研究

 多输入多输出(MIMO)雷达是近年来出现的一种新体制雷达,针对MIMO体制的机载雷达开展空时自适应处理（STAP）技术研究是值得进一步努力的方向。本文研究了机载MIMO雷达STAP技术的降维算法,通过对STAP技术杂波抑制原理进行分析,推导并得到一种基于杂波子空间的降维算法。结合扁长椭球波函数（PSWF）的特点,提出了一种基于杂波子空间估计的降维算法,并与若干降维算法的杂波抑制性能进行比较。结果表明,当存在阵元幅相误差时,该算法在保持杂波抑制性能的同时能够有效地降低STAP算法的运算量。     

一种简单的自适应延迟补偿方法

针对模型参考自适应控制对延迟鲁棒性较差的问题,提出了将动态特性接近被控对象的参考模型作为前馈补偿器,从而改进系统性能的补偿方法。仿真结果表明,该补偿方法效果明显,且对不确定的延迟扰动有一定的鲁棒性。     

光电跟踪仪激光测距器性能检测方法研究

介绍了光电跟踪仪激光测距器的特点,提出了其重要性能指标一测距能力和精度的检测方法。采用半实物仿真技术测试反映测距能力的消光比参量;采用精密延时法,实现了测距精度的测量。检测装置的耦合透镜部件放置于平行光管靶面,容易与测试光电跟踪设备其它模块的装置进行集成。     

时空一致性对武器系统仿真试验影响的分析

时空一致性是影响仿真试验精度的最为关键的重要因素之一。文章阐述了由于时钟不同步导致的对时间和空间理解的不一致,以及对仿真精度的影响,详细分析了时空不一致产生的各种可能因素,并以某型武器系统仿真试验为例,提出了几种实用且可行的时空一致性处理方法。     

Multi-agent Q-Learning control of spacecraft formation flying reconfiguration trajectories

This paper presents a novel approach based on multi-agent reinforcement learning for spacecraft formation flying reconfiguration tracking problems. In this scheme, spacecrafts learn the control strategy via transfer learning. For this matter, a new generalized discounted value function is introduced for the tracking problems. Due to the digital nature of spacecraft computer systems, local optimal controllers are developed for the spacecrafts in discrete-time. The stability of the controller is proven. Two Q-learning algorithms are proposed, in each of which the optimal control solution is learned on-line without knowledge about the system dynamics. In the first algorithm, each agent learns the optimal control independently. In the second one, each agent shares the learned information with other agents. Next, the collision avoidance capability is provided. The effectiveness of the presented schemes is verified through simulations and compared with each other.     

基于小波神经网络的PIM功率时间序列预测

无源互调（passive intermodulation,PIM）是影响通信系统性能的关键因素之一。研究表明,PIM信号并非一个定值,而是随时间变化的非平稳信号。基于PIM功率信号的时间序列特性,文章提出基于小波神经网络的PIM功率时间序列预测方法。首先,详细介绍小波神经网络预测模型及其预测方法;其次,以同轴连接器为验证对象,通过PIM实验测试系统获得3阶PIM功率的时间序列;最后,依据获得的PIM功率时间序列,结合构建的小波神经网络预测模型对后续的时间序列进行预测分析,并将预测结果与实验结果进行比较,从而验证小波神经网络在预测PIM功率时间序列方面的有效性。该研究对于开展PIM抑制技术具有一定的参考价值。     

Optimal steering law of refractive sail

The interaction between electromagnetic waves and matter is the working principle of a photon-propelled spacecraft, which extracts momentum from the solar radiation to obtain a propulsive acceleration. An example is offered by solar sails, which use a thin membrane to reflect the impinging photons. The solar radiation momentum may actually be transferred to matter by means of various optical phenomena, such as absorption, emission, or refraction. This paper deals with the novel concept of a refractive sail, through which the Sun’s light is refracted by crossing a film made of polymeric micro-prisms. The main feature of a refractive sail is to give a large transverse component of thrust even when the sail nominal plane is orthogonal to the Sun-spacecraft line. Starting from the recent literature results, this paper proposes a semi-analytical thrust model that estimates the characteristics of the propulsive acceleration vector as a function of the sail attitude angles. Such a mathematical model is then used to analyze a simplified Earth-Mars and Earth-Venus interplanetary transfer within an optimal framework.