一种临近空间高超声速飞行器翼舵干扰研究

在临近空间区域内飞行的高超声速飞行器对舵面操纵特性提出了严苛的要求,在高空高速条件下主翼对舵效有严重影响。通过风洞试验对带全动舵升力体的高超声速升阻特性进行了研究,发现由于主翼的遮挡效应,负舵偏比同舵偏值的正舵偏对升力体升阻特性影响更明显。数值模拟结果显示在舵偏角从-20°～20°变化过程中,由于主翼与舵面之间气流干扰造成舵面上下压差变化复杂,-12°～2°舵偏产生抬头铰链力矩,其余正负舵偏均产生低头铰链力矩,主翼后缘上表面的分离线随攻角增加逐渐前移,迎风面高压气流通过翼舵之间缝隙向上发展,使得舵上表面再附线后移,翼舵之间均有明显的横向流动。     

人工拉格朗日点附近的被动稳定飞行

利用太阳帆能在三体问题中实现人工拉格朗日点,人工拉格朗日点克服了经典拉格朗日点位置固定的缺点,研究人工拉格朗日点的被动控制对深空探测有重要的意义。理论上人工拉格朗日点都不稳定,研究表明在被动控制下存在某些人工拉格朗日点的稳定特性与稳定平衡点非常接近,在工程上可以认为稳定。被动控制可以通过设计太阳帆来实现,本文给出了被动稳定太阳帆的设计,在该设计下考虑轨道和姿态的耦合动力学方程。基于该耦合方程研究了人工拉格朗日点的稳定性。仿真结果表明被动太阳帆使得人工拉格朗日点稳定。     

我校大学生心理健康状况不容乐观

本文用SCL－90症状自评量表方法，对我校三个年级的部分班级进行了测查。分析表明：我院大学生的心理健康状况不容乐观。本文还对学生管理现状提出了进一步改进建议。     

多体卫星复合控制物理仿真试验系统

对于具有星间链路天线的多体卫星而言 ,进行星体姿态和天线指向复合控制的地面物理仿真试验研究是一个重要课题。本文主要叙述利用单轴气浮台模拟卫星姿态运动 ,由天线框架驱动机构 (GDA)实物连接组成的多体卫星平面运动动力学环境下的物理仿真试验系统。     

基于矢量测量和UKBF的飞越小天体自主导航方法研究

以估计航天器和小天体在日心惯性系中的位置和速度为目的,提出了基于视线矢量测量的飞越小天体自主导航方法。该方法利用导航相机和激光高度计构建航天器到目标天体的视线矢量,同时为避免系统方程线性化和离散化所带来的模型误差,采用UKBF (Unscented Kalman\|Bucy Filter)算法对相应位置和速度进行估计。分析了导航系统的能观性,并以坦普尔一号为目标天体进行仿真验证,理论分析和仿真结果皆表明了方法的有效性和可行性。
     

基于GM(1,1)分段组合的宽体货机预测模型研究

航空货运市场是全球航空运输市场的重要组成部分,与全球经济、贸易的发展息息相关。航空货运市场的发展趋势及需求直接影响到货机市场的发展趋势及货机行业的发展规划。而作为全球航空货运市场的运输载体,货机尤其是远程宽体货机对货物的国际间运输和交流起到了至关重要的作用。当前主流的预测方法为根据需求与供应的对应关系进行预测,预测过程相对复杂,预测的精度相对较高,不足之处在于预测工作周期较长,难以快速获得预测的结果。根据当前灰色系统理论,建立了宽体货机机队预测的灰色预测模型GM(1,1),并用分段组合的方式,较为精确地预测宽体货机未来机队的发展情况,预测较为快速,效率较高,能满足一般精度的预测需求。     

运动的核弹比静止的核弹威力小?——多普勒效应、红移、光行差和动体的质能当量关系

证明爱因斯坦立足于光速不变假设和长度收缩假设的洛伦茨变换未能正确地解释多普勒效应、红移和光行差现象;他也未能给出正确的动体的质能当量关系.作者立足于完全符合相对性原理的伽利略变换,成功地解决了上述问题.     

椭球台高杆灯风荷载的实验研究

通过风洞实验研究了多钝体高杆灯在不同水平风向角和竖向风向角下的力与力矩系数。实验结果表明在一定的风向角下，法向阻力系数Cdmax=1.030,法向弯曲力矩系数Cmmax=-0.940,轴向力系数Camax=0.504和Camin=-0．600。     

Dynamics of a spacecraft and normalization around Lagrangian points in the Neptune–Triton system

The problem of a spacecraft orbiting the Neptune–Triton system is presented. The new ingredients in this restricted three body problem are the Neptune oblateness and the high inclined and retrograde motion of Triton. First we present some interesting simulations showing the role played by the oblateness on a Neptune’s satellite, disturbed by Triton. We also give an extensive numerical exploration in the case when the spacecraft orbits Triton, considering Sun, Neptune and its planetary oblateness as disturbers. In the plane a × I (a = semi-major axis, I = inclination), we give a plot of the stable regions where the massless body can survive for thousand of years. Retrograde and direct orbits were considered and as usual, the region of stability is much more significant for the case of direct orbit of the spacecraft (Triton’s orbit is retrograde). Next we explore the dynamics in a vicinity of the Lagrangian points. The Birkhoff normalization is constructed around L₂, followed by its reduction to the center manifold. In this reduced dynamics, a convenient Poincaré section shows the interplay of the Lyapunov and halo periodic orbits, Lissajous and quasi-halo tori as well as the stable and unstable manifolds of the planar Lyapunov orbit. To show the effect of the oblateness, the planar Lyapunov family emanating from the Lagrangian points and three-dimensional halo orbits are obtained by the numerical continuation method.     

A Structured Mesh Euler and Interactive Boundary Layer Method for Wing/Body Configurations

To compute transonic flows over a complex 3D aircraft configuration, a viscous/inviscid interaction method is developed by coupling an integral boundary-layer solver with an Eluer solver in a ＂semi-inverse＂ manner. For the turbulent boundary-layer, an integral method using Green＇s lag equation is coupled with the outer inviscid flow. A blowing velocity approach is used to simulate the displacement effects of the boundary layer. To predict the aerodynamic drag, it is developed a numerical technique called far-field method that is based on the momentum theorem, in which the total drag is divided into three component drags, i.e. viscous, induced and wave-formed. Consequently, it can provide more physical insight into the drag sources than the often-used surface integral technique. The drag decomposition can be achieved with help of the second law of thermodynamics, which implies that entropy increases and total pressure decreases only across shock wave along a streamline of an inviscid non-isentropic flow. This method has been applied to the DLR-F4 wing/body configuration showing results in good agreement with the wind tunnel data.