基于脑电和眼动信号的人机交互意图识别

意图识别在人机交互（HCI）领域受到广泛关注,传统人机交互意图识别方法单纯依靠脑电（EEG）或眼动数据,不能很好地利用2种方法优点。为此,提出了一种融合脑电和眼动数据的人机交互意图识别方法,通过采集脑电和眼动信号,进行特征提取,输入机器学习模式识别网络进行意图识别,并基于Dempster-Shafer （D-S）证据理论进行决策层融合得出最终识别结果。招募了20名有效受试者进行交互意图识别实验,结果表明,基于脑电和眼动信号的人机交互意图识别方法识别准确率高于单纯依靠脑电和眼动数据的方法,可为下一步飞行器和武器系统人机交互系统自适应设计提供理论依据和技术支持。     

小天体附近的轨道动力学研究综述

小天体附近的轨道动力学是现代天体力学的一个重要研究方向,包含着丰富的物理现象和深刻的数学内涵;随着一系列小行星实地探测任务的深入开展,理解小天体附近的轨道运动规律也成为航天领域所面对的众多挑战之一。回顾了小天体研究和探测的历程,分析了小天体附近轨道动力学问题的基本特点和科学价值;详细介绍了航天动力学、行星学和非线性科学三个学科领域对该问题的讨论和研究进展,并列举了各领域中相关的热点问题;基于对上述研究现状的分析,尝试展望了该研究方向未来的发展趋势。     

基于星间距离测量的高精度自主导航

研究利用地球卫星和月球卫星之间的测距信息进行自主导航的方法.基于三体摄动轨道动力学方程和星间测距信息,可以同时确定参与导航的地球卫星和月球卫星的绝对位置;但是在初始位置误差较大的情况下,导航系统的定位性能会受到影响.为了解决这一问题,提出基于"星间测距+紫外导航敏感器"的组合导航方法.采用该导航方法,能够在初始位置误差和紫外导航敏感器测量误差较大的情况下实现高精度自主导航.基于Cramer-Rao下界(CRLB)分析了组合导航系统的性能,并通过数学仿真验证了该导航方法的有效性.     

Theoretical and Experimental Analysis on Influence of Revolution Radius in Orbital Drilling

Revolution radius is one of the significant parameters in orbital drilling,which has great influence on many factors,such as the cutting area of front and side cutting edge,undeformed chip geometry,delamination and burr at hole exit side,hole surface roughness,cutting tool force and deflection,chip removal and heat transmission.First,the influence of revolution radius on the factors is discussed theoretically in detail.Analysis results show that big revolution radius can reduce axial cutting force,restrain exit delamination and burr,and improve chip removal and heat transmission.Then,single factor test and orthogonal test are utilized in the two processing methods as machining unidiameter holes with several cutting tools and machining different diameter holes with one tool.Finally,the influence of revolution radius on cutting force and hole machining precision is studied.These results provide a profound foundation for future optimization of cutting control parameters.     

Real-time evaluation method of flight mission load based on sensitivity analysis of physiological factors

As the complexity of flight missions continues to increase, sending a timely warning or providing assistance to pilots helps to reduce the probability of operational errors and flight accidents. Monitoring pilots’ physiological data, real-time evaluation of mission load is a feasible technical way to achieve this. In this paper, a set of flight tasks including aircraft control, humancomputer interaction and mental arithmetic tests are designed to simulate five mission loads at different flight d...     

Water movement on the convex surfaces of porous media under microgravity

A plant growth system for crop production under microgravity is part of a life supporting system designed for long-duration space missions. A plant growth in soil in space requires the understanding of water movement in soil void spaces under microgravity. Under 1G-force condition, on earth, water movement in porous media is driven by gradients of matric and gravitational potentials. Under microgravity condition, water movement in porous media is supposed to be driven only by a matric potential gradient, but it is still not well understood. We hypothesized that under microgravity water in void spaces of porous media hardly moved comparing in void spaces without obstacles because the concave surfaces of the porous media hindered water movement. The objective of this study was to investigate water movement on the convex surfaces of porous media under microgravity. We conducted parabolic flight experiments that provided 20–25?s of microgravity at the top of a parabolic flight. We observed water movement in void spaces in soil-like porous media made by glass beads and glass spheres (round-bottomed glass flasks) in the different conditions of water injection under microgravity. Without water injection, water did not move much in neither glass beads nor glass spheres. When water was injected during microgravity, water accumulated in contacts between the particles, and the water made thick fluid films on the particles surface. When the water injection was stopped under microgravity, water was held in the contacts between the particles. This study showed that water did not move upward in the void spaces with or without the water injection. In addition, our results suggested that the difficulty of water movement on the convex (i.e. particle surfaces) might result in slower water move in porous media under microgravity than at 1G-force.     

基于PnP和自适应线性卡尔曼滤波的实时位姿估计

针对实时位姿估计中扩展卡尔曼滤波(EKF)线性化引入非线性误差和依赖已知噪声分布的缺点,提出一种基于PnP的自适应线性卡尔曼滤波位姿估计求解方法。将PnP位姿估计求解策略引入卡尔曼滤波观测方程,通过对动态方程误差统计参数实时估计,自适应调节卡尔曼滤波递推参数。所提算法求解精度高,固定了观测方程的观测向量维度,提高了算法实用性。通过仿真试验,比较了该算法与EKF的位姿估计精度,通过量化误差分析,证明了该方法可以提高三维运动位姿估计精度,也验证了该方法的有效性。     

重力姿轨耦合效应引起的太阳能电站轨道共振

以任意相控阵天线式空间太阳能电站为研究对象,主要研究了其在轨运行过程中受到的重力姿轨耦合效应对其轨道运动的影响。首先,通过Hamilton原理建立起考虑重力姿轨耦合效应时的姿态运动和轨道运动的方程。其中,任意相控阵天线式空间太阳能电站被简化成刚体,它的重力势能以其结构尺寸和其轨道半径的比值为小量进行泰勒展开,并保留至二阶项。之后,采用解析的方法对方程进行分析,并发现当电站的姿态运动满足一定条件时,其轨道运动将会出现共振现象。此外,重力姿轨耦合效应还会引起空间太阳能电站轨道运动长期的漂移,通过选择合适的轨道运动初始条件可以消除漂移;而且,在一定条件下,重力姿轨耦合效应还会引起轨道运动的发散。最后,数值仿真结果验证了分析的正确性。     

现代小卫星的发展及轨道垃圾问题

文章首先综述半个多世纪以来传统和现代小卫星的技术发展,特别是现代小卫星在对地观测、通信导航、空间技术实验与演示、深空探测、军事等方面的应用取得很多成就,尤其是对地观测高分辨率成像系统取得了突破性技术成就;其次讨论小卫星所产生的轨道垃圾及其影响和处理;最后提出未来小卫星技术发展十个原则,对未来小卫星的应用作了展望。     

增强型轨道列表星历及其在北斗混合星座中的应用

为了改进北斗卫星数小时内的力模型精度,分析日月引力摄动和光压摄动的短期变化特性,提出基于二次多项式逼近日月引力摄动的15参数增强型轨道列表星历模型。利用该星历模型对北斗的5 GEO + 5 IGSO + 4 MEO混合星座进行了为期11天的星历拟合实验。结果表明,三类卫星在非地影期的2小时星历拟合精度优于1 cm。增强型轨道列表星历模型没有轨道根数的潜在奇点问题,能够为我国北斗星座和星基增强系统提供更多可行的星历模型选择。