椭圆振动切削加工的同步控制研究

利用椭圆振动切削加工的回转体表面微织构是在机床主轴旋转、平台进给和装置椭圆振动的联合运动下得到的,机床主轴转动与装置位移输出如果不能保持完全的实时同步,会造成微织构加工的偏差。为了解决这一问题,提出了一种新的基于转角的同步控制方法,该方法在主轴的对位基准处实现装置正弦信号的复位,以修正转速漂移造成的加工位置误差,并通过判断主轴角度信号实时输出对应幅值电压来实时同步信号输出和机床旋转运动。基于LabVIEW FPGA搭建同步控制模块,经试验验证,利用该方法加工的矩形阵列微织构轴向排列与中轴线平行,与周向排列的夹角和仿真结果的偏差不超过0.1°,织构深度随转角的不同发生预设的变化,因此,同步控制方法具有实时同步控制椭圆振动切削装置的能力。     

考虑捷联导引头最小视场角约束的制导策略

针对高超声速飞行器捷联导引头，提出导引头最小视场角（FOV）约束问题。首先分析了导引头视线角变化规律，指出在攻击固定目标时，导引头最小视场角约束在弹道末段无法被满足，导引头将丢失目标。在此基础上，基于缩短导引头丢失目标距离的目标，提出一种满足导引头最小视场角约束的制导策略。该策略不依赖于末制导律形式，当最小视场角约束无法被满足时，改变原有制导指令，主动改变弹道轨迹以增加弹体视线角，避免超出视场范围。其次，针对飞行器过载约束，设计了制导策略切换点，在到达切换点时该制导策略将结束工作，避免末端过载过大超出约束。通过对比仿真验证了所提出制导策略有效性，能够大幅度减少导引头丢失目标距离，工程上有利于提高末端命中精度。     

对于动态目标的航天器鲁棒PD+快速跟踪控制方法

摘要：针对卫星对于空间动态目标快速、稳定地跟踪、控制目标，同时考虑平台模型的不确定性、外部随机干扰、系统控制力矩与角速度约束等因素，设计PD+控制器实现对于动态目标的快速、稳定跟踪；在经典PD控制器的基础上设计控制添加项使得系统能够按照既定轨迹运动；采用变结构的手段实现系统收敛速度的提升；合理设计Lyapunov函数的结构，引出角速度、四元数的耦合项对V函数进行改良，简化系统稳定性证明与分析的过程；讨论系统最极端情形，通过对V函数上下界的讨论分析系统该情形下的稳定性；最后通过数值仿真验证所提出算法的有效性与优越性.     

超精密微牛级微波离子推进技术及其在卫星超精度控制中的应用研究

空间技术的快速发展使得利用空间卫星的编队飞行构建大型空间星座成为可能，在引力波探测、射电望远镜编队、星座组网等任务方面具有重要作用。超精度控制是实现卫星高精度编队飞行的关键技术。推进系统是实现卫星编队长期高度稳定飞行的保证，从而实现内部科学装置的正确运行。不同于常规的推进系统，卫星精密编队超精度控制对推进系统的推力可调范围、分辨率、响应时间、推力的一致性等有着极高的要求。根据卫星精密编队任务需求，对微牛级推进系统的功能及技术要求进行了分析，提出了基于M2微波离子推力器的卫星超精度控制推进系统。阐述了M2超精密微牛级推进系统的关键技术和研究进展，为后续M2推力器在无拖曳控制方面的应用奠定了基础。     

带攻角约束的高超声速飞行器自适应反步控制器设计

针对带攻角(AOA)约束的高超声速飞行器控制问题，提出一种基于非对称时变障碍函数的非线性自适应反步控制方法。首先，将飞行器模型化为严反馈形式，以反步法为基础进行控制器设计。然后通过光滑饱和函数对名义攻角指令信号进行限幅，并保证限幅信号的可导性，限幅产生的误差通过设计辅助系统进行补偿。进而使用障碍函数对攻角指令跟踪误差进行非对称时变约束。针对不确定性和干扰，设计新型自适应律对集中干扰上界进行估计并补偿。最终通过Lyapunov理论证明了闭环系统状态量一致最终有界并且攻角始终满足时变约束。仿真结果表明，本文方法能够在满足攻角约束基础上保证良好跟踪性能。     

Event-triggered attitude control of spacecraft

The problem of spacecraft attitude stabilization control system with limited communication and external disturbances is investigated based on an event-triggered control scheme. In the proposed scheme, information of attitude and control torque only need to be transmitted at some discrete triggered times when a defined measurement error exceeds a state-dependent threshold. The proposed control scheme not only guarantees that spacecraft attitude control errors converge toward a small invariant set containing the origin, but also ensures that there is no accumulation of triggering instants. The performance of the proposed control scheme is demonstrated through numerical simulation.     

Neural adaptive control for a ground experiment of the space proximity operation in a six-degree-of-freedom micro-gravity simulation system

In this study, a neural adaptive controller is developed for a ground experiment with a spacecraft proximity operation. As the water resistance in the experiment is highly nonlinear and can significantly affect the fidelity of the ground experiment, the water resistance must be estimated accurately and compensated using an active force online. For this problem, a novel control algorithm combined with Chebyshev Neural Networks (CNN) and an Active Disturbance Rejection Control (ADRC) is proposed. Specifically, the CNN algorithm is used to estimate the water resistance. The advantage of the CNN estimation is that the coefficients of the approximation can be adaptively changed to minimize the estimation error. Combined with the ADRC algorithm, the total disturbance is compensated in the experiment to improve the fidelity. The dynamic model of the spacecraft proximity maneuver in the experiment is established. The ground experiment of the proximity maneuver that considers an obstacle is provided to verify the efficiency of the proposed controller. The results demonstrate that the proposed method outperforms the pure ADRC method and can achieve close-to-real-time performance for the spacecraft proximity maneuver.     

Application of improved active disturbance rejection control algorithm in tilt quad rotor

The Tilt Quad Rotor (TQR) has complex dynamics characteristics, especially in conversion mode. It is difficult to build the dynamic model of the TQR and the environmental factors have a great influence on it. To solve the problem of control in conversion mode of TQR, this paper carries out the design of the controller based on improved Active Disturbance Rejection Control (ADRC). According to the characteristics of flight in conversion mode, Tracking Differentiator (TD) with explicit model is used to solve the problem of multiple integrals when the system is high-order system. Extended State Observer (ESO) with Radial Basis Function (RBF) neural network is used to estimate and compensate for internal and external uncertainties, and the adaptive sliding mode control in Nonlinear State Error Feedback (NLSEF) is used to improve the response speed of the controller and reduce the parameters which should be tuned. Through the flight control simulation of the TQR, the validity and rationality of the control system are verified.     

航天器姿态大角度机动有限时间控制

针对航天器姿态大角度机动控制问题，在存在外部扰动的情况下，基于航天器姿态跟踪系统的标准级联特性，利用反步法和自适应控制设计有限时间控制器。提出的控制方法可以严格保证姿态大角度机动系统是全局有限时间稳定的。李雅普诺夫理论推导和仿真结果表明，系统在控制器的作用下可以快速机动到平衡点并保持稳定，全物理仿真试验进一步表明了所提出的控制方法的有效性和优越性。     

Statistical characteristics of low latitude Pc4s: Influence of solar wind and IMF parameters

Pc4 signatures for the year 2013, extracted from geomagnetic north–south and east–west components of induction coil magnetometer (LEMI 30) from low latitude station Desalpar (DSP), operated by Institute of Seismological Research (ISR), India have been investigated vis-à-vis the prevalent interplanetary parameters (IMF) as well as the geomagnetic activity indices. A clear dominance of Pc4-5 (467 events) over Pc3 (17 events) is observed. Local time variation of Pc4 shows a peak in the noon sector in both X and Y components. Our investigations show that the dominant peak frequency is 10 mHz at low latitude region. Correlations with solar wind and IMF parameters illustrate highest occurrence of Pc4 for a solar wind speed of 300–400 km/s and average IMF B field of 3–6 nT. The amplitude of Pc4s at DSP shows an increase with increasing solar wind speed, plasma density, solar wind dynamic pressure and average B field which is also reflected in the trend of frequency variation of these pulsations. We report that IMF clock angle at low latitude does not have influence on Pc4 occurrence. Based on the characteristics of these events, detected in latitudinally distributed stations from low and mid-latitudes from northern and southern hemisphere, we infer that modes were compressional, which could be driven by K-H instability or solar wind dynamic pressure, as compressional modes can propagate to low latitude with little attenuation.