同平面LEO-LEO气动辅助空间交会

给出了实现同平面LEO-LEO空间交会的必要条件，分析了基于脉冲的主动调相方法，并重点研究了基于气动辅助轨道转移技术实现同平面LEO—LEO的空间交会方案。通过设计标准的同平面HEO—LEO气动辅助轨道转移最优轨迹，得到OTV与目标实现交会必须满足的标准相角，然后采用主动调相法使飞行器运行到高轨道时，恰好满足HEO—LEO气动辅助空间交会的标准相角，最后借助气动辅助轨道转移技术实现空间交会。该方法具有扩大发射窗口，且比基于脉冲主动调相法节省燃料等优点。     

Optimal deployment schedule of an active twist rotor for performance enhancement and vibration reduction in high-speed flights

The best active twist schedules exploiting various waveform types are sought taking advantage of the global search algorithm for the reduction of hub vibration and/or power required of a rotor in high-speed conditions.The active twist schedules include two non-harmonic inputs formed based on segmented step functions as well as the simple harmonic waveform input.An advanced Particle Swarm assisted Genetic Algorithm (PSGA) is employed for the optimizer.A rotorcraft Computational Structural Dynamics (CSD) code CAMRAD Ⅱ is used to perform the rotor aeromechanics analysis.A Computation Fluid Dynamics (CFD) code is coupled with CSD for verification and some physical insights.The PSGA optimization results are verified against the parameter sweep study performed using the harmonic actuation.The optimum twist schedules according to the performance and/or vibration reduction strategy are obtained and their optimization gains are compared between the actuation cases.A two-phase non-harmonic actuation schedule demonstrates the best outcome in decreasing the power required while a four-phase non-harmonic schedule results in the best vibration reduction as well as the simultaneous reductions in the power required and vibration.The mechanism of reduction to the performance gains is identified illustrating the section airloads,angle-of-attack distribution,and elastic twist deformation predicted by the present approaches.     

Ferrofluid moving thin films for active flow control

Ferrofluid moving thin films and their possible significance with regard to active flow control for lift and attack angle enhancement are discussed. In this strategy, a very thin film of ferrofluid is strongly attached at the wall of the wing by a normal magnetic field from below and pumped tangentially along the wing. Utilizing a simplified physical model and from the available experimental data on moving walls, the expected lift enhancement and effect on the attack angle were assessed. Additional research and design is required in order to explore the possibilities in the use of ferrofluid moving thin films.     

三轴稳定微小卫星主动磁阻尼姿态控制

针对三轴稳定微小卫星,用四元数法建立了速率阻尼阶段的动力学和运动学模型.根据地磁场强度矢量投影到轨道坐标系的简便旋转关系,设计了采用主动磁控的拟比例微分控制器,同时分析了磁力矩器的磁偶极矩.速率阻尼仿真结果表明:该控制法有效可行,具有一定的应用价值.     

合成射流激励器实验及结果分析

设计了合成射流激励器及实验测试系统。对两大小不同激励器工作于不同驱动频率及激励电源电压幅值分别进行了实验，并对激励器出口速度进行了分析。实验测得的合成射流出口最大峰值速度可达5m／s，驱动频率对激励器出口射流速度影响直接明显，且合成射流激励器有工作频谱范围限制。通过频谱分析显示，只有最大峰值频率与激励频率相等或接近，而且各峰值频率与最大峰值频率成倍频关系时，合成射流激励器将电能转化为合成射流动能的效率才能达到较高。     

基于空间交会的天基反卫作战方案

对位于高地球轨道天基平台攻击低地球轨道目标的方案进行了研究,讨论了高轨作战平台的攻击范围。采用完全推力法实现远程空间交会。为消除异面霍曼变轨方法等待时间过长的缺点,提出了两种主动调相方法。研究表明：用该法可实现天基武器由高轨至低轨的空间转移交会,引入主动调相轨道可明显缩短交会所需时间。     

采用分布式压电驱动器的翼面热颤振主动抑制

高超声速气动加热会严重影响飞行器结构的颤振特性,本文开展了采用分布式压电驱动器的热颤振主动抑制方法研究。以某飞行器小展弦比翼面为研究对象,进行了常温和热载荷边界条件下的结构振动和颤振分析。在此基础上,对频域非定常气动力进行有理函数拟合,建立包含压电驱动器的翼面耦合结构系统状态空间形式的运动方程;对典型热载荷边界条件下的被控对象设计颤振主动抑制控制律,分别设计出LQG及PID控制器;对比分析了系统开、闭环颤振特性。结果表明,通过主动控制律的实施,达到了热颤振主动抑制的目的,验证了这种颤振主动抑制方法的有效性     

Dark energy,co-evolution of massive black holes with galaxies,and ASTROD-GW

The detection of low frequency band (100 nHz–100 mHz) and very low frequency band (300 pHz–100 nHz) gravitational waves (GWs) is important for exploration of the equation of state of dark energy and the co-evolution of massive black holes (MBHs) with galaxies. Most galaxies are believed to have a massive black hole in the galactic core. In the formation of these black holes, merging and accretion are the two main processes. Merging of massive black holes generate GWs which could be detected by space GW detectors and Pulsar Timing Arrays (PTAs) to cosmological distances. LISA (Laser-Interferometric Space Antenna) is most sensitive to the frequency band 1 mHz–100 mHz, ASTROD-GW (ASTROD [Astrodynamical Space Test of Relativity using Optical Devices] optimized for Gravitational Wave detection) is most sensitive to the frequency band 100 nHz–1 mHz and PTAs are most sensitive to the frequency band 300 pHz–100 nHz. In this paper, we discuss the sensitivities and outlooks of detection of GWs from binary massive black holes in these frequency bands with an emphasis on ASTROD-GW. The GWs generated by the inspirals, merging and subsequent ringdowns of binary black holes are standard sirens to the cosmological distance. Using GW observations, we discuss the methods for determining the equation of state of dark energy and for testing the co-evolution models of massive black holes. ASTROD-GW is an optimization of ASTROD to focus on the goal of detection of GWs. The mission orbits of the 3 spacecraft forming a nearly equilateral triangular array are chosen to be near the Sun-Earth Lagrange points L3, L4 and L5. The 3 spacecraft range interferometrically with one another with arm length about 260 million kilometers. With 52 times longer in arm length compared to that of LISA, the strain detection sensitivity is 52 times better toward larger wavelength. The scientific aim is focused for gravitational wave detection at low frequency. The science goals include detection of GWs from MBHs, and Extreme-Mass-Ratio Black Hole Inspirals (EMRI), and using these observations to find the evolution of the equation of state of dark energy and to explore the co-evolution of massive black holes with galaxies.     

Fuzzy multi-criteria decision-making approach to prioritization of space debris for removal

As private companies and government space agencies begin to seriously consider the task of active space debris removal, it is becoming increasingly more important to determine the highest priority objects to deorbit. This work sets forth an approach for prioritization of space debris through the utilization of Multi-Criteria Decision-Making methodologies and fuzzy logic, as well as both quantitative and qualitative criteria. The proposed debris prioritization approach considers various criteria including the orbit, size, mass, pairwise and total collision probabilities, and decay timeframe of each debris object. The means of assigning attributes to each assessment criterion is discussed in detail. To determine the weighting scheme for the criteria, a questionnaire was prepared and shared with experts in the field of space situational awareness. The work examines over two thousand critical debris objects selected from the existing debris catalog with respect to these criteria. The quantified attributes for each debris object are then aggregated through the fuzzy versions of the Analytic Hierarchy Process and the Technique for Order Preference by Similarity to Ideal Solution. The results of the analysis identify high-priority debris objects for removal from Earth-bound orbits.