多个自由飞行空间机器人协调操作运动规划

本文提出了在空间微重力环境下多个自由飞行空间机器人协调操作运动规划算法，首先推导出多个自由飞行空间机器人协调操作的广义雅可比矩阵，其次给出了基于该矩阵的多个自由飞行空间机器人协调操作分解运动速度控制算法，最后用计算机仿真验证了该算法的正确性。     

Cascade-type guidance law design for multiple-UAV formation keeping

A procedure to compute guidance commands for controlling the relative geometry of multiple unmanned aerial vehicles (UAVs) in formation flight is proposed. The concepts of branch, global leader, and local leader/follower are used to represent the whole formation geometry. A positive-definite function defined in terms of the formation error is then introduced and the Lyapunov stability theorem is used to obtain the cascade type guidance law. This scheme leads to the synchronized flight of all UAVs while maintaining formation geometry. The results of a high fidelity nonlinear simulation of a reconnaissance and surveillance mission example are presented to show the effectiveness of the proposed guidance law.     

舰载机飞行员驾驶技术与飞行安全研究

针对无法将驾驶技术和飞行安全建立有效定量关联的现状,基于自适应飞机驾驶员最优控制模型,应用飞行员着舰多层次模糊综合评价方法,通过设定不同的飞行员模型参数,参照着舰技能评价体系,建立了飞行员着舰技能样本库.通过多元非线性回归方法,建立了飞行员技能的多元非线性回归模型,并通过剩余标准差和样本比对法证明了这一模型的准确性.可以通过测定上述飞行员参数,运用该飞行技能回归模型,为飞行员选拔提供参考.     

小展弦比飞翼亚、跨、超声速支撑干扰研究

通过数值模拟方法研究了小展弦比飞翼标模在0.6、0.9、1.5三个典型马赫数下的支撑干扰特性,分别考虑了近场尾部外形局部畸变和尾支杆干扰及远场风洞中部支架干扰,并基于表面压力系数差异为准则尝试对近场干扰量进行分解。研究得到如下结论:马赫数0.6时,远场支撑阻力系数和俯仰力矩系数的干扰量约占总支撑干扰量的30%,升力系数约占20%;马赫数0.9、迎角2°时,阻力系数远场支撑干扰量占总支撑干扰量的40%,迎角18°时,远场支撑干扰使得涡破裂位置提前;马赫数1.5时,远场支撑干扰可以忽略;基于表面压力系数差异将支撑干扰量分解的方法在亚声速支撑干扰前传明显时不适用,在马赫数0.9、迎角2°时求得近场支撑干扰使得马赫数减小约0.02,迎角减小约0.1°,马赫数1.5时用此法求得马赫数和迎角的干扰量均约等于0。     

自由飞行空间机器人基座位姿调整的模糊PD控制

由于自由飞行空间机器人处于微重力的环境,因此其在目标获取的过程中必然会出现因机械臂运动和环境影响而导致基座的复杂运动.本文设计了自由飞行空间机器人位姿调整的模糊PD算法,根据接收到的实时位置信息,空间机器人可以自主地调整基座的姿态和位置来校正位姿误差,保证目标的稳定捕获.利用开发的实验平台与传统的on/off式控制器进行了实验对比,验证了此方法在稳定性、控制精度和燃料消耗上都有较好的表现.     

Stability and shape analysis of relative equilibrium for three-spacecraft electromagnetic formation

The invariant shapes for close formation flying with inter-craft electromagnetic force ensure several potential space applications. However, the 6-DOF relative equilibrium problem has not been systematically investigated. This paper mainly analyzes the invariant shapes of relative equilibrium for the three-spacecraft electromagnetic formation, and studies the families of invariant shape solutions with real and constant magnetic moments as well as their linear stability. The problem is examined based on the full nonlinear coupled dynamic models for collinear and general triangular configurations. The relative equilibrium conditions are analyzed to determine whether an invariant shape do exist, and the corresponding families of invariant shape solutions are identified for static and spinning configurations respectively. Finally, the linear stability of such invariant shapes is numerically discussed, which have shown that most invariant shapes are unstable and controllable.     

卫星编队飞行相对轨道主被动结合测量方案研究

针对军用编队飞行卫星系统相对轨道测量隐蔽性要求，提出一种具有隐蔽性的主被动结合相对位置及速度测量方案，该方案采取激光测距仪间断工作的方式以减少向外界辐射能量。应用扩展kalman滤波算法，对编队卫星间相对位置及速度进行估计，并且采用计算可观测度方法对系统可观测性进行分析。滤波计算及可观测性分析结果表明该方案满足一定测量精度，验证了该方案的有效性，使该方案具有工程应用价值。     

ISO Observations of Pre-Stellar Cores and Young Stellar Objects

We summarize the observations of the Infrared Space Observatory (ISO) concerning the earliest stages of the stellar formation. The observations of samples of sources in different evolutionary stages are reviewed, addressing in particular how the physical and chemical properties of the protostellar environments change from the pre-stellar cores to the protostars at the end of their accretion phase. In addition, the mid-IR surveys in nearby star-forming regions are discussed, showing their implications for the understanding of the stellar initial mass function. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

Low ionization lines in high luminosity quasars: The calcium triplet

In order to investigate where and how low ionization lines are emitted in quasars we are studying a new collection of spectra of the CaII triplet at λ8498, λ8542, λ8662 observed with the Very Large Telescope (VLT) using the Infrared Spectrometer And Array Camera (ISAAC). Our sample involves luminous quasars at intermediate redshift for which CaII observations are almost nonexistent. We fit the CaII triplet and the OI λ8446 line using the Hβ profile as a model. We derive constraints on the line emitting region from the relative strength of the CaII triplet, OI λ8446 and Hβ.     

Effective Coulomb force modeling for spacecraft in Earth orbit plasmas

Coulomb formation flight is a concept that utilizes electrostatic forces to control the separations of close proximity spacecraft. The Coulomb force between charged bodies is a product of their size, separation, potential and interaction with the local plasma environment. A fast and accurate analytic method of capturing the interaction of a charged body in a plasma is shown. The Debye–Hückel analytic model of the electrostatic field about a charged sphere in a plasma is expanded to analytically compute the forces. This model is fitted to numerical simulations with representative geosynchronous and low Earth orbit (GEO and LEO) plasma environments using an effective Debye length. This effective Debye length, which more accurately captures the charge partial shielding, can be up to 7 times larger at GEO, and as great as 100 times larger at LEO. The force between a sphere and point charge is accurately captured with the effective Debye length, as opposed to the electron Debye length solutions that have errors exceeding 50%. One notable finding is that the effective Debye lengths in LEO plasmas about a charged body are increased from centimeters to meters. This is a promising outcome, as the reduced shielding at increased potentials provides sufficient force levels for operating the electrostatically inflated membrane structures concept at these dense plasma altitudes.