基于3层结构的新一代航管信息系统的设计与实现

采用3层结构理论对新一代航管信息系统进行了设计,并对系统研制中的关键技术,包括3层结构的物理实现、基于部件的应用开发、OLE、WindowsSocket、数据实时同步和访问控制等的实现方法进行了分析研究,最后给出了系统的应用实例。     

双机斤斗飞行中上赶下掉问题的研究

简述了飞机斤斗飞行的基本运动关系和操纵动作要领。以双纲斤斗为例，指出了双机编队复杂特技科目中存在着突出的上赶下掉现象；并阐明了上赶下掉现象形成的原因及其特点。重点探讨了保持双机斤斗编队距离的操纵方法、基本原理和具体修正计算式。最后，为保证飞行安全，分析了双机斤斗飞行易出现的主要偏差、特殊情况、修正方法以及应注意的有关问题。     

Understanding Galaxy Formation with ISO Deep Surveys

We present the results obtained through the various ISO extragalactic deep surveys. Although IRAS revealed the existence of galaxies forming stars at a rate of a few tens (LIRGs) or even hundreds (ULIRGs) solar masses in the local universe, ISO not only discovered that these galaxies were already in place at redshift one, but also that they are not the extreme objects that we once believed them to be. Instead they appear to play a dominant role in shaping present-day galaxies as reflected by their role in the cosmic history of star formation and in producing the cosmic infrared background detected by the COBE satellite in the far infrared to sub-millimeter range. 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.     

MHD numerical simulations of proto-stellar jets

We will summarize in this paper the effects that the presence of the magnetic field can cause to proto-stellar jet dynamics, structure and emission line properties, and the differences between two- and three-dimensional numerical simulations will be emphasized. This revised version was published online in August 2006 with corrections to the Cover Date.     

基于零空间方法的四旋翼无人机避障与协同编队控制

针对四旋翼无人机在编队飞行执行任务时可能遭遇障碍物问题,考虑多无人机避障及机间避撞的需求,提出 1种基于零空间方法的四旋翼无人机避障与协同编队控制算法。首先,建立四旋翼无人机动力学模型,并建立虚拟控制量简化控制模型;其次,基于零空间方法进行避障与协同编队控制算法研究,将无人机任务执行分解为目标趋向任务、避障避撞任务和协同编队任务,并根据优先级进行任务融合得到期望速度;再次,基于 PID方法设计控制律;最后,通过仿真验证所提控制算法的有效性。所提方法可保证四旋翼无人机在编队飞行中遭遇障碍物时的飞行安全。     

Design and optimization of stable initial heliocentric formation on the example of LISA

Space-based gravitational wave (GW) detector such as the LISA (Laser Interferometer Space Antenna) mission requires high-precision and stability of the triangular formation. The dynamic environment of the detectors is complex, the science requirements for the formation are tight, and consequently, design and optimization of this high-standard formation with essentially many decision variables are very challenging. This paper studies the design and optimization of the stable initial formation of the heliocentric GW detector by taking the LISA as an example. The linearization method based on relative orbital elements is used for formation design in the two-body system. Three constraints are presented to reduce the number of decision variables to fourteen. The geometric features of the arm length and breathing angle of the triangular formation and the relative position of LISA to the Earth are analyzed and numerically verified in a high-fidelity dynamic model, from which the relationships of multiple requirements of LISA are studied, and a single index is summarized to simplify the optimization. Sobol sensitivity analysis is used to quantitatively evaluate the sensitivities of the decision variables to the cost function, with which a self-adaptive adjustment algorithm of the region of the variables is presented to improve the computational efficiency. The availability of the method to quickly and precisely find a stable initial formation in an extensive neighborhood of the nominal formation is verified by numerical simulation, where the best solution decreases about 47.54% of the arm length change from the requirement. This study shows that the initial formation should be deployed appropriately away from the Earth, and the gravitations of Venus and Jupiter should be utilized to maintain the formation stability.     

Integrated orbit and attitude hardware-in-the-loop simulations for autonomous satellite formation flying

Development and experiment of an integrated orbit and attitude hardware-in-the-loop (HIL) simulator for autonomous satellite formation flying are presented. The integrated simulator system consists of an orbit HIL simulator for orbit determination and control, and an attitude HIL simulator for attitude determination and control. The integrated simulator involves four processes (orbit determination, orbit control, attitude determination, and attitude control), which interact with each other in the same way as actual flight processes do. Orbit determination is conducted by a relative navigation algorithm using double-difference GPS measurements based on the extended Kalman filter (EKF). Orbit control is performed by a state-dependent Riccati equation (SDRE) technique that is utilized as a nonlinear controller for the formation control problem. Attitude is determined from an attitude heading reference system (AHRS) sensor, and a proportional-derivative (PD) feedback controller is used to control the attitude HIL simulator using three momentum wheel assemblies. Integrated orbit and attitude simulations are performed for a formation reconfiguration scenario. By performing the four processes adequately, the desired formation reconfiguration from a baseline of 500–1000 m was achieved with meter-level position error and millimeter-level relative position navigation. This HIL simulation demonstrates the performance of the integrated HIL simulator and the feasibility of the applied algorithms in a real-time environment. Furthermore, the integrated HIL simulator system developed in the current study can be used as a ground-based testing environment to reproduce possible actual satellite formation operations.     

PBO合成、纺丝和性能的研究

以间苯二酚为原料，合成了单体4，6-二氨基间苯二酚二盐酸盐，在多聚磷酸介质中经溶液缩聚，制得高分子量的聚亚苯基苯并二噁唑（PBO），再由干喷湿纺工艺制备了PBO纤维，并对纤维成型工艺以及热处理条件进行了研究。结果表明，PBO纤维的拉伸强度为4．31GPa、拉伸模量为117．24GPa，它是一种高性能的刚性溶致性液晶高分子材料。     

复合材料层合板多向层间的Ⅱ型分层断裂韧性研究

 <正> 1.引言 近年来,用断裂力学方法研究复合材料的分层破坏成为复合材料力学的一个热点。自1985年Russell提出用端部开口弯曲(简称为ENF)试样测量单向层间的Ⅱ型分层断裂韧性的方法以来,关于单向层间的Ⅱ型分层断裂问题已经得到较为充分的     

小卫星编队飞行队形设计与轨道要素确定

用两体相对运动的线性Hill方程进行了小卫星编队飞行队形的初步设计，并给出编队飞行中各绕飞小卫星轨道要素的确定过程，以空间圆形编队为例，在未考虑摄动情况下，通过仿真验证了Hill方程在小卫星编队队形初步设计中的有效性。