机匣转静刮磨后轴流压气机气动性能评估研究

为揭示机匣可磨耗涂层磨损造成的叶尖间隙和粗糙度变化对压气机气动性能的影响规律,针对不同刮磨形貌下Rotor 37转子性能进行了数值模拟研究。结果表明,压气机等熵效率和出口流量对刮磨间隙和粗糙度的变化较为敏感,降幅最高可达1.78%和0.83%,而压比变化不大;刮磨间隙深度增加,刮磨最深位置前移时,叶尖泄漏增强,泄漏流与上端壁附面层及主流相互作用演变为泄漏涡,与激波相互干涉,造成较大的叶尖损失;压气机气动性能受磨损区域粗糙度影响较小,虽然等熵效率对粗糙度变化较为敏感,但最大降幅也仅为0.38%。磨损区域粗糙度增加时,近壁区湍流波动加强且气流更易分离,引起叶尖泄漏流和叶片尾迹区域的流动结构变化,使压气机气动特性向低流量方向偏移。     

转子-基础系统的随机不确定建模与振动分析

以具有基础弹性支承的Jeffcott转子为研究对象,并考虑到外部随机激励对基础的作用和转定子间的碰摩现象,建立了带碰摩故障的转子-基础随机外激励系统的动力学微分方程.应用相应的数值仿真方法,给出了该系统随外部随机激励变化影响下的轴心轨迹、频谱图和Poincaré图等;分析了随机外激励的变化对转子-基础系统的影响.结果表明随机外激励强度和谱宽的变化以及周期外激励频率的改变将引起振动模式(如频率和波形等)的改变,并将导致转子出现周期、倍周期和混沌等复杂的动力学行为.      

无人直升机任务规划系统研究与实践

无人直升机任务规划系统对于完成超视距侦察、监控能力和打击是非常重要的.本文分析了无人直升机任务规划系统的的基本体系结构和功能模块,研究了无人直升机任务规划系统的建模技术及其优化算法,并在V750无人直升机上进行了验证.     

标准轨迹制导中准平衡滑翔条件优化研究

对于可重复使用运载器标准轨迹再入制导,准平衡滑翔条件可以将高度-速度平面内各项再入约束形成的飞行走廊,转换为倾侧角-速度空间内的倾侧角走廊.通过在倾侧角走廊内设计倾侧角曲线,可以生成满足飞行走廊的标准轨迹.通过论证标准轨迹再入制导过程中的准平衡滑翔条件及其物理意义,说明了由倾侧角走廊内的倾侧角曲线生成的标准轨迹,存在突破再入飞行走廊边界的可能性.通过对倾侧角走廊边界设置余度,极大地降低了标准轨迹突破再入飞行走廊边界的可能性,提高了标准轨迹的设计成功率.     

A fast arc fault detection method for AC solid state power controllers in MEA

Arc fault detection is desperately required in Solid State Power Controllers (SSPC) in addition to their fundamental functions because arcs will provoke growing harm and threat to aircraft safety. Experimental study has been done to obtain the faulted current data. In order to improve the detection speed and accuracy, two fast arc fault detection methods have been proposed in this paper with the analysis of only half cycle data. Both Fast Fourier Transform (FFT) and Wavelet Packets Decomposition (WPD) have been adopted to distinguish arc fault currents from normal operation currents. Analysis results show that Alternating Current (AC) arcs can be effectively and accurately detected with the proposed half cycle data based methods. Moreover, experimental verification results have also been provided.     

Relative position and attitude estimation of spacecrafts based on dual quaternion for rendezvous and docking

The capacity to acquire the relative position and attitude information between the chaser and the target satellites in real time is one of the necessary prerequisites for the successful implementation of autonomous rendezvous and docking. This paper addresses a vision based relative position and attitude estimation algorithm for the final phase of spacecraft rendezvous and docking. By assuming that the images of feature points on the target satellite lie within the convex regions, the estimation of the relative position and attitude is converted into solving a convex optimization problem in which the dual quaternion method is employed to represent the rotational and translational transformation between the chaser body frame and the target body frame. Due to the point-to-region correspondence instead of the point-to-point correspondence is used, the proposed estimation algorithm shows good performance in robustness which is verified through computer simulations.     

Cosmic-ray propagation through the disturbed heliosphere

The stationary, source-free, one-dimensional solution to the cosmic-ray heliospheric transport equation was solved using Runge–Kutta methods. These calculations have been applied to the treatment of Forbush decreases and the evolution of the solar cycle through the heliosphere. Forbush decreases calculated by this method produce spectra that are in good agreement with both the theoretical heliocentric potential and the potential as determined from neutron monitor data. During solar modulation, the effect of the travelling disturbance is to flatten the gradient of the cosmic ray flux in the inner heliosphere at solar minimum and steepen the gradient at solar maximum, as the incoming cosmic rays see solar activity up to a year earlier. The resulting spectra at the earth's orbit are in good agreement with the heliocentric approximation. The heliocentric approximation is an accurate and convenient method of accounting for solar modulation.     

Solar-photon sail hovering orbits about single and binary asteroids

Solar-photon sails can be useful for missions towards and about asteroids. Indeed, for the interplanetary transfer phase, missions to asteroids often require a large variation in inclination and solar-photon sails perform very well for such high energy missions. In the same way, solar-photon sails are also expected to perform well in the phase about the asteroid. This paper studies single and binary asteroids’ hovering regions by using a sailcraft. In order to consider a sailcraft with its own mass and shape, the mutual polyhedral method (usually used to study asteroid dynamics) is used; therefore, the sailcraft is designed by means of tetrahedra. The procedure to obtain the hovering regions about a single asteroid is presented and an accurate analysis of the control variables is carried out. Moreover, control torques required to maintain hovering orbits are obtained by considering the gravitational torques acting on the sailcraft due to the asteroid. In the end, the theory for hovering orbits is extended to binary-asteroid systems and applied to the binary system 1999 KW4.     

执行器饱和的多智能体一致性控制

针对执行器饱和约束下的一类离散多智能体系统，设计了一种基于线性矩阵不等式的一致性控制律，并对线性矩阵不等式解的存在性进行了分析。由于饱和环节的影响，导致多智能体系统的一致性与个体的初始状态有关，不同的控制律所能允许的个体之间的初始偏差的范围不同。为了定量分析控制律所对应的初始偏差范围，引入吸引域的概念对所设计的控制律进行评估，并对控制律参数进行优化以扩大吸引域的范围。最后，通过数值仿真说明了所设计控制律的有效性。     

Spacecraft formation-containment flying control with time-varying translational velocity

This paper investigates the problem of Spacecraft Formation-Containment Flying Control (SFCFC) when the desired translational velocity is time-varying. In SFCFC problem, there are multiple leader spacecraft and multiple follower spacecraft and SFCFC can be divided into leader spacecraft’s formation control and follower spacecraft’s containment control. First, under the condition that only a part of leader spacecraft can have access to the desired time-varying translational velocity, a velocity estimator is designed for each leader spacecraft. Secondly, based on the estimated translational velocity, a distributed formation control algorithm is designed for leader spacecraft to achieve the desired formation and move with the desired translational velocity simultaneously. Then, to ensure all follower spacecraft converge to the convex hull formed by the leader spacecraft, a distributed containment control algorithm is designed for follower spacecraft. Moreover, to reduce the dependence of the designed control algorithms on the graph information and increase system robustness, the control gains are changing adaptively and the parametric uncertainties are handled, respectively. Finally, simulation results are provided to illustrate the effectiveness of the theoretical results.