空间站维修性系统设计与验证方法研究

空间站在轨运行时间长,因此需采用维修性设计和在轨维修的方法实现长寿命高可靠在轨运行。根据维修性设计理论,结合工程实际,提出了基于产品特性分析的维修需求分析方法和维修支持下的可靠度计算方法。明确了系统维修性设计应包括布局、供电、信息、故障检测、维修工作模式等设计内容。并根据维修难度,提出了四级维修策略。最后根据在轨维修特点,提出了地面试验验证和仿真验证的方法。为空间站系统维修性设计提供了一个技术途径。     

刀具声发射信号混沌特征提取及趋势分析

旨在建立一种基于多混沌特征演化分析的刀具磨损状态监测方法,通过计算刀具声发射信号的混沌特性参数分析其磨损趋势。建立首先基于混沌理论分析和描述刀具不同磨损阶段声发射信号的混沌特性,包括：定性描述,即重构相空间的奇异吸引子轨迹和庞加莱截面;定量描述,计算不同时间段声发射信号的关联维数、最大Lyapunov指数等。其次,采用最小二乘回归方法对所计算的混沌参数进行趋势分析。结果表明,声发射信号具有混沌特性,而且关联维数和最大Lyapunov指数演化趋势与刀具的磨损状态具有一定的关联,从而为刀具磨损状态的在线监测和预测提供了新思路。     

基于相空间重构的网络流量RBF神经网络预测

应用混沌理论,分析了网络流量,用单变量的网络流量时闯序列重构与网络动力系统等距同构的相空间,进而计算了实际网络的关维数和Lyapunov指数,并证实了网络流量存在混沌特性;据此建立了基于径向基函数（RBF）神经网络的模型,并对实际网络数据流进行了预测。仿真结果表明,相对于其他前馈神经网络预测,基于混沌理论的RBF神经网络预测方法学习速度快,预测精度高。     

基于光纤F-P可调谐滤波器的有害气体检测方法

光谱分析法在气体成分监测领域有着广泛的应用,实现小型紧凑高分辨率的光谱测量装置是热门的研究课题。文章创造性的提出了基于光纤法布里-帕罗（F—P）的可调谐滤波器提高吸收光谱分辨率,为构建紧凑高分辨率的光谱仪提供了一种新的方案。基于光纤F-P的可调谐滤波器成功实现了微型光栅光谱仪（分辨率约1nm）对甲烷吸收光谱的测量,对比无光纤F—P可调谐滤波器直接测量的结果,该方法测得的吸收光谱强度至少提高了一个数量级。此研究成果可用于紧凑高分辨率的星载气体检测仪的研制。     

国外多模式霍尔电推进发展概况及启示

多模式霍尔电推进具有多个工作模式,调节能力强,相对于20世纪80年代以来广泛应用的只有一个工作模式的霍尔电推进器,其优势明显,能很好地适应诸如GEO卫星轨道转移和在轨位置保持,以及深空探测器和空间运输平台的主推进等多种任务,因此得到了广泛研究和应用.国外多模式霍尔电推进发展现状和趋势对我国多模式霍尔电推进的发展具有重要的启示作用.针对我国航天器对电推进的迫切任务需求,定量分析应用多模式霍尔电推进的收益,提出我国多模式霍尔电推进发展的建议.     

多关节轻型机械臂的设计研究

根据现有空间机械臂的结构特点,参照几种轻型机械臂的设计,设计了一种两自由度机械臂运动模块,并根据此模块研制了一台6自由度空间机械臂。运动模块由两个相邻关节轴线正交的关节组成,关节内部没有驱动器。机械臂内有一根高速主轴,为各个串联关节提供动能。机械臂控制系统采用上下位机方式,上位机根据虚拟场景仿真的运动轨迹发出控制指令给关节控制器,下位机根据关节状态表控制离合器组输入关节的能量。为确定机械臂在工作过程中的强度和稳定性,建立了机械臂的有限元模型,分析了其工作态的应力情况和动态特性。仿真结果表明,机械臂在工作态有足够的强度,在抓取的过程中,机械臂固有频率远离激励源的激励频率,无共振现象。通过多关节联动,机械臂可实现多种组合姿态,适用于在轨维修、加注等复杂空间任务。     

Deep Impact: Working Properties for the Target Nucleus – Comet 9P/Tempel 1

In 1998, Comet 9P/Tempel 1 was chosen as the target of the Deep Impact mission (A’Hearn, M. F., Belton, M. J. S., and Delamere, A., Space Sci. Rev., 2005) even though very little was known about its physical properties. Efforts were immediately begun to improve this situation by the Deep Impact Science Team leading to the founding of a worldwide observing campaign (Meech et al., Space Sci. Rev., 2005a). This campaign has already produced a great deal of information on the global properties of the comet’s nucleus (summarized in Table I) that is vital to the planning and the assessment of the chances of success at the impact and encounter. Since the mission was begun the successful encounters of the Deep Space 1 spacecraft at Comet 19P/Borrelly and the Stardust spacecraft at Comet 81P/Wild 2 have occurred yielding new information on the state of the nuclei of these two comets. This information, together with earlier results on the nucleus of comet 1P/Halley from the European Space Agency’s Giotto, the Soviet Vega mission, and various ground-based observational and theoretical studies, is used as a basis for conjectures on the morphological, geological, mechanical, and compositional properties of the surface and subsurface that Deep Impact may find at 9P/Tempel 1. We adopt the following working values (circa December 2004) for the nucleus parameters of prime importance to Deep Impact as follows: mean effective radius = 3.25± 0.2 km, shape – irregular triaxial ellipsoid with a/b = 3.2± 0.4 and overall dimensions of ∼14.4 × 4.4 × 4.4 km, principal axis rotation with period = 41.85± 0.1 hr, pole directions (RA, Dec, J2000) = 46± 10, 73± 10 deg (Pole 1) or 287± 14, 16.5± 10 deg (Pole 2) (the two poles are photometrically, but not geometrically, equivalent), Kron-Cousins (V-R) color = 0.56± 0.02, V-band geometric albedo = 0.04± 0.01, R-band geometric albedo = 0.05± 0.01, R-band H(1,1,0) = 14.441± 0.067, and mass ∼7×10¹³ kg assuming a bulk density of 500 kg m⁻³. As these are working values, {i.e.}, based on preliminary analyses, it is expected that adjustments to their values may be made before encounter as improved estimates become available through further analysis of the large database being made available by the Deep Impact observing campaign. Given the parameters listed above the impact will occur in an environment where the local gravity is estimated at 0.027–0.04 cm s⁻² and the escape velocity between 1.4 and 2 m s⁻¹. For both of the rotation poles found here, the Deep Impact spacecraft on approach to encounter will find the rotation axis close to the plane of the sky (aspect angles 82.2 and 69.7 deg. for pole 1 and 2, respectively). However, until the rotation period estimate is substantially improved, it will remain uncertain whether the impactor will collide with the broadside or the ends of the nucleus.     

Calculation of the transonic dip of airfoils using viscous-inviscid aerodynamic interaction method

A numerical procedure for the calculation of the transonic dip of airfoils in the time domain is presented. A viscous-inviscid aerodynamic interaction method is taken to calculate the unsteady aerodynamic loads. In the present case the integral boundary layer equations are coupled with the Transonic Small Disturbance (TSD) Potential Equation. The coupling between structural motion and aerodynamic loads is carried out using State Space equation. It is solved by State Transition Matrix technique. Results are presented for NACA 64A010 and NLR 7301 airfoils with structural data from Isogai and DLR, respectively. Comparisons show good agreement with other numerical results. Certain deviations of experimental data taken from literature need more insight in the detailed test conditions.     

深空通信中LDPC码的一种译码算法

LDPC码由于具有逼近仙农极限的性能和硬件可实现的编译码复杂度,在深空通信中具有重要的应用前景。文章在简要介绍CCSDS（空间通信系统咨询委员会）中LDPC码编码规范的基础之上,采用多维EXIT图对其译码门限和收敛速度进行了研究,最后重点研究了译码算法,通过改进归一化最小和算法提出了一种自适应归一化最小和算法,该算法保留了归一化最小和算法的所有优点,改善了不同信噪比条件下的译码性能,并解决了归一化因子的选择难题,适合在资源受限的深空通信中应用。
     

航天器相对导航与控制技术的典型任务

在空间交会对接、在轨服务、近距离目标监视以及航天器编队飞行任务中,通常需要通过相对导航与控制技术对相互邻近的航天器进行控制.回顾了该领域典型的空间任务,特别关注任务、相对导航与控制方法、相对测量设备、推进系统等主要特征,并总结了该项技术的发展趋势.