基于单轴随机扩展算法的自主探测器大角度机动规划

自主姿态大角度机动是自主深空探测器的关键技术之一，而在满足敏感仪器、保持通信链路等约束的情况下实现姿态大角度机动的自主规划与执行是目前面临的一个难题。针对这个问题，提出一种单轴随机扩展算法，该算法采用扩展的方式生成规划路径，并充分利用扩展过程中邻近点的信息，把属于三维构造空间的大角度机动规划问题简化为二维规划问题，从而减少问题求解的搜索空间。最后利用前向搜索方法对初始的规划路径进行优化，并通过算例验证了此方法的可行性。     

Ares V launch vehicle: An enabling capability for future space science missions

NASA's planned Ares V cargo launch vehicle offers the potential to completely change the paradigm of future space science mission architectures. Future space science telescopes desire increasingly larger telescope collecting aperture. But, current launch vehicle mass and volume constraints are a severe limit. The Ares V greatly relaxes these constraints. For example, while current launch vehicles have the ability to place a 4.5 m diameter payload with a mass of 9400 kg on to a Sun-Earth L2 transfer trajectory, the Ares V is projected to have the ability to place an 8.8 m diameter payload with a mass of approximately 60,000 kg on to the same trajectory, or 180,000 kg into Low Earth Orbit. Also the Ares V could place approximately 3000 kg (13,000 kg with a Centaur upper stage) on to a trajectory with a C3 of 106 km²/s², arriving at Saturn in 6.1 years without the use of gravity assists. This paper summarizes the current planned Ares V payload launch capability.     

Numerical analysis of broadband noise reduction with wavy leading edge

Large Eddy Simulation(LES) is performed to investigate the airfoil broadband noise reduction with wavy leading edge under anisotropic incoming turbulence. The anisotropic incoming turbulence is generated by a rod with a diameter of 10 mm. The incoming flow velocity is 40 m/s and the corresponding Reynolds numbers based on airfoil chord and rod diameter are about 397000 and 26000, respectively. The far-field acoustic field is predicted using an acoustic analogy method which has been validated by the experiment. A straight leading edge airfoil and a wavy leading edge airfoil are simulated. The results show that wavy leading edge increases the airfoil lift and drag whereas the lift and drag fluctuations are substantially reduced. In addition, wavy leading edge can significantly change the flow pattern around the leading edge and a pair of counter-rotating streamwise vortices stemming from each wavy leading edge peak are observed.An averaged noise reduction of 9.5 dB is observed with the wavy leading edge at the azimuthal angle of 90°. Moreover, the wavy leading edge can mitigate noise radiation at all the azimuthal angles without significantly changing the noise directivity. The underlying noise reduction mechanisms are then analyzed in detail.     

Very large space structures: Non-linear control and robustness to structural uncertainties

Very Large Space Structures (VLSS) are challenging systems to be controlled, due to their high flexibility. In particular, rapid attitude maneuvers can determine great oscillations on the flexible elements of a spacecraft (solar wings, antennas, booms). On account of this, in the last decades many researchers have developed different strategies to effectively damp the elastic vibrations by means of active vibration devices (such as piezo-electric patches) or by means of robust control algorithms. The approach suggested in this paper is different, since neither additional devices nor complex control laws are introduced. In fact, the complete model of the system (including rigid, elastic and orbital dynamics, coupled with control actions) is controlled by the non-linear attitude controller named state dependent Riccati equation, which will be based on a simplified version of the spacecraft model. The task to reduce the mutual interaction between rigid attitude and flexible dynamics is entirely transferred to a modification of the desired trajectory that must be tracked. This command shaping technique is based on the knowledge of the parameters (inertial and elastics) of the VLSS. Unfortunately these parameters are not always exactly known and, however, they may change over the time. On account of this a Monte Carlo analysis has been also performed, showing the robustness of the proposed control strategy to the structural uncertainties. The numerical simulations prove that this strategy, based on the joint application of two well-known yet simple techniques, produces accurate and robust results.     

一种基于三维到达角的无偏伪线性卡尔曼滤波

为了解决大场景下基于三维到达角的目标跟踪问题，提出了一种具有无偏性的伪线性卡尔曼滤波。首先，基于三维到达角信息对目标运动模型与量测模型进行建模；之后，对量测模型进行了伪线性化处理，得到了线性形式的目标量测模型。为了解决伪线性卡尔曼滤波存在的有偏性问题，提出了一种结合EKF（extend Kalman filter）的三维伪线性无偏卡尔曼滤波。仿真实验表明，该模型能够对非机动目标与机动目标有效跟踪，对于百公里级别的目标，当角测量误差从0.1°变化到0.5°，算法在仿真时间结束时均能将绝对位置误差降低至10 km以内，且算法的运行速度与EKF为同一个量级，同时兼顾了抗干扰能力、定位跟踪精度、运行效率的要求，能够为大场景下的目标跟踪提供有效方法。     

大尺度空气舵超声速烧蚀热结构试验

针对全尺寸大尺度空气舵热环境参数,对地面试验的流场参数进行了计算,设计了测试探头,进行了流场校测。将校测结果与计算结果进行了比较分析,结果表明二者吻合较好,最大偏差在30%以内。校测后的流场已成功应用于试验。     

大负荷低压涡轮叶型分离转捩流动的大涡模拟

应用动力模式大涡模拟数值方法,对来流无扰动、不可压、雷诺数为5×104(基于进口速度和轴向弦长),定常来流条件下大负荷低压涡轮叶型(Pak B)叶型吸力面非定常分离转捩流动进行了三维数值模拟。在与相关实验数据的对比基础之上,对非定常流动物理信息进行了详细的分析讨论,揭示了计算来流状态下的Pak B叶型吸力面非定常分离转捩流动机理。结果表明,由无粘Kelvin-Helmholtz机制产生的、空间线性增长的初始二维不稳定性在分离剪切内诱导展向旋涡形成并脱落,脱落过程中的展向涡在非线性增长的三维不稳定性作用下发生变形并最终破碎成湍流。计算得到的Kelvin-Helmholtz不稳定性特征频率处于相关实验测量范围内。     

大尺寸弧长图像测量系统及其图像处理方法的研究

基于CCD图像测量技术,提出一种新的非接触大尺寸弧长图像测量系统,该系统可用于测量封闭或非封闭、规则或不规则轮廓的大尺寸弧长。文中给出了系统的结构及原理,并着重讨论了该系统的图像处理方法。最后,利用新系统进行了现场比对实验。     

Surface accuracy analysis of large deployable antennas

This paper performs an analysis to the systematic surface figure error influenced by three factors including errors of faceted paraboloids, fabrication imperfection and random thermal strains in orbit. Firstly, the computational formulas for root-mean-square surface deviations caused by these factors are presented respectively. The stochastic finite element method is applied to derive the computational formulas of fabrication imperfection and random thermal strains, by which the sensitivity of surface accuracy to component imperfection can be revealed. Then the Monte Carlo simulation method is introduced to obtain the surface figure by sampling test on random errors. Finally, the analytical method is applied to the research on the surface figure error of AstroMesh deployable reflector. The results show that the deviations between the root-mean-square surface errors calculated by the proposed formulas with less consuming time and those by the Monte Carlo simulation method are less than 2%, which indicates that the proposed method is efficient and receivable enough to analyze systematic surface figure error of a large deployable antenna. Moreover, further investigations on the relationship between surface RMS deviation and the antenna parameters including aperture and the number of subdivisions are presented in the end.     

一种带导引头视角和落角约束的导引方法

针对导弹大落角需求下引起的目标超出导引头视场造成锁定失败的情况,提出了一种采用开关逻辑的导引律。该方法在落角控制导引律的基础上引入了一个开关项,当导引头视角超出设定阈值时开启开关项,通过反向原指令加速度来抑制视角的增大,使目标始终处在导引头视场之内,当导引头视角小于设定阈值时关闭开关项以发挥原导引律的优势。新导引律能有效攻击固定与运动目标,且无需弹目相对距离信息。仿真表明,该导引律既有效地限制了导引头视角,又保留了原导引律高落角精度和指令加速度在末段收敛到零的特性。