无人机栖落机动建模与轨迹优化

对固定翼无人飞行器栖落机动的纵向运动进行了气动特性建模与轨迹优化设计。通过运动捕捉系统测量获得试验滑翔机实时飞行数据,并结合统计学原理和平板气动理论建立了气动模型和动力学模型。针对所建立的模型采用GPOPS优化工具箱设计了栖落机动标称轨迹。优化结果表明,不同初始速度条件下执行栖落机动的空间需求不同,但最终都可以实现以相同的栖落速度落到同一位置。     

冲压空气涡轮释放过程运动学分析

冲压空气涡轮作为飞机上的应急能源,能在出现紧急情况时提供电能,保证飞机上电传操控和电子设备的正常工作。本文以冲压空气涡轮为研究对象,基于机械运动原理对系统模型进行了简化,基于刚体假设,结合MATLAB软件从理论上研究结构在释放过程中的运动学问题。给出了冲压空气涡轮系统释放过程中各个关节空间位置的理论求解方法,得到了关节在空间中的运动轨迹和对应的速度时间曲线、加速度时间曲线,结果表明:冲压空气涡轮系统的释放过程在1 s以内,释放速度较快,且各关节在释放初始阶段速度、加速度响应较大。本文的工作可为后期不同冲压空气涡轮系统构型的初步设计提供理论依据,指导冲压空气涡轮释放的仿真计算和试验。     

航天器相对运动建模及周期性相对运动求解

面向航天器编队飞行的需求,对椭圆参考轨道航天器非线性周期相对运动条件进行研究,提出了确定椭圆参考轨道编队航天器非线性周期性相对运动条件的新方法。首先,考虑非线性、椭圆轨道等因素,通过哈密尔顿-雅可比(HJ)方程和正则摄动理论,推导了在任意非线性摄动下相对运动的模型和获得不需消耗任何燃料的周期性相对运动轨道的条件;然后,采用时域配点法,结合改进的列文伯格-马夸尔特(LM)法对周期性相对运动的初值进行求解;最后,设计数值仿真算例,利用上述条件,得到不消耗任何燃料的周期性绕飞轨道,由此验证了本文所提模型和方法的正确性。     

Friction moment analysis of space gyroscope bearing with ribbon cage under ultra-low oscillatory motion

This paper presents the model of calculating the total friction moment of space gyroscope ball bearings which usually work under ultra-low oscillatory motion and are very sensitive to the friction moment. The aim is to know the proportion of the friction moment caused by each frictional source in the bearing＇s total friction moment, which is helpful to optimize the bearing design to deduce the friction moment. In the model, the cage dynamic equations considering six degree-of-freedom and the balls dynamic equations considering two degree-of-freedom were solved.The good trends with different loads between the measured friction moments and computational results prove that the model under constant rate was validated. The computational results show that when the speed was set at 5 r/min, the bearing＇s maximum total friction moment when oscillation occurred was obviously larger than that occurred at a constant rate. At the onset of each oscillatory motion, the proportion of the friction moment caused by cage in the bearing＇s total friction moment was very high, and it increased with the increasing speed. The analyses of different cage thicknesses and different clearances between cage pocket and ball show that smaller thickness and clearance were preferred.     

多种失效模式相关的机构运动可靠度计算方法

机构运动中必然存在多种相关失效模式,多为影响机构运动的各类随机变量函数.为了在机构运动可靠性分析中有效考虑多种相关失效模式的影响,建立了考虑多种失效模式相关条件下的机构运动可靠度计算模型,并实现了对多种失效模式相关条件下的机构运动可靠度计算模型的求解,为考虑多种相关失效模式下的机构运动可靠性分析提供了一种有效途径.以6408滚动轴承为例,进行100 000抽样计算,考虑失效模式相关条件下运动可靠度为95.998 9%.该方法精度较高,具有一定的理论意义和应用价值.     

虚拟座舱环境头颈部sEMG采集相关肌肉研究

针对虚拟座舱环境下飞行员头部运动实时准确检测问题,在对头部运动特性进行分析的基础上,系统性地总结了人体头颈部sEMG信号采集的相关研究文献。针对头部突然旋转和俯仰运动,通过实验验证已有的sEMG信号采集方法,确定了利用sEMG信号进行头部运动检测时所需要研究的肌肉及准确的肌肉位置标识以及电极放置方法。     

张力腿漂浮式风力机的运动响应计算

漂浮式风力机与近海桩基式风力机、陆上风力机差异很大,特别是漂浮平台设计复杂,对仿真工具要求更高。海上风力机除受气动载荷之外,还需进一步考虑海洋环境所施加的各种其他载荷。采用自由涡尾迹方法计算风力机气动性能,分别采用线性波和PM频谱模拟波浪运动并应用Morison方程计算波浪载荷。构建张力腿漂浮平台结构动力学方程,以气动载荷和波浪载荷为激励,得到平台响应,并反馈至气动计算,从而完成气动、结构和水动的耦合计算。最后以大型风力机NH1500为例,对张力腿式海上风力机进行仿真模拟,对比分析来流风速、浪高和波浪入流角对漂浮平台运动和风力机气动性能的影响,采用PM频谱模拟真实海况并计算漂浮式风力机动态响应,为漂浮式风力机设计提供了依据。     

IDS contribution to ITRF2008

For the first time, the International DORIS Service (IDS) has produced a technique level combination based on the contributions of seven analysis centers (ACs), including the European Space Operations Center (ESOC), Geodetic Observatory Pecny (GOP), Geoscience Australia (GAU), the NASA Goddard Space Flight Center (GSFC), the Institut Géographique National (IGN), the Institute of Astronomy, Russian Academy of Sciences (INASAN, named as INA), and CNES/CLS (named as LCA). The ACs used five different software packages to process the DORIS data from 1992 to 2008, including NAPEOS (ESA), Bernese (GOP), GEODYN (GAU, GSC), GIPSY/OASIS (INA), and GINS (LCA). The data from seven DORIS satellites, TOPEX/Poseidon, SPOT-2, SPOT-3, SPOT-4, SPOT-5, Envisat and Jason-1 were processed and all the analysis centers produced weekly SINEX files in either variance–covariance or normal equation format. The processing by the analysis centers used the latest GRACE-derived gravity models, forward modelling of atmospheric gravity, updates to the radiation pressure modelling to improve the DORIS geocenter solutions, denser parameterization of empirically determined drag coefficients to improve station and EOP solutions, especially near the solar maximum in 2001–2002, updated troposphere mapping functions, and an ITRF2005-derived station set for orbit determination, DPOD2005. The CATREF software was used to process the weekly AC solutions, and produce three iterations of an IDS global weekly combination. Between the development of the initial solution IDS-1, and the final solution, IDS-3, the ACs improved their analysis strategies and submitted updated solutions to eliminate troposphere-derived biases in the solution scale, to reduce drag-related degradations in station positioning, and to refine the estimation strategy to improve the combination geocenter solution. An analysis of the frequency content of the individual AC geocenter and scale solutions was used as the basis to define the scale and geocenter of the IDS-3 combination. The final IDS-3 combination has an internal position consistency (WRMS) that is 15 to 20 mm before 2002 and 8 to 10 mm after 2002, when 4 or 5 satellites contribute to the weekly solutions. The final IDS-3 combination includes solutions for 130 DORIS stations on 67 different sites of which 35 have occupations over 16 years (1993.0–2009.0). The EOPs from the IDS-3 combination were compared with the IERS 05 C04 time series and the RMS agreement was 0.24 mas and 0.35 mas for the X and Y components of polar motion. The comparison to ITRF2005 in station position shows an agreement of 6 to 8 mm RMS in horizontal and 10.3 mm in height. The RMS comparison to ITRF2005 in station velocity is at 1.8 mm/year on the East component, to 1.2 mm/year in North component and 1.6 mm/year in height.     

有磁场时电子在航天器光电子鞘层中的漂移运动

采用二级漂移近似理论，研究了在航天器光电子鞘层中与电流收集有关的电子在磁场中的运动轨道和收集电子有关的磁瓶结构，结果表明当磁场越强，航天器表面电势越弱，磁瓶在无穷远处横截面积就越小。在光电子鞘层中，势垒对电流收集影响较大，磁瓶的横截面积在略远于垫垒处有极大值，磁瓶在无穷远处的横截面积并非随着势垒距航天器距离的远近而单调变化。     

Periodic relative orbits of two spacecraft subject to differential gravity and electrostatic forcing

Coulomb forces between charged close-flying satellites can be used for formation control, and constant electric potentials enable static equilibria solutions. In this work, open-loop time-varying potential functions, which produce periodic, two-craft, Coulomb formation motions are demonstrated for the first time. This is done in the rotating Hill-Frame, with linearized gravity, and craft position components assumed in the form of simple harmonic oscillators. Substitution of the oscillatory functions into the dynamics, further constrains these functions, and yields necessary potential histories, to produce the periodic flow. The assumed position functions, however, are not arbitrary, since the dynamical model restricts what oscillatory trajectories are allowed. Specifically, a Hill-Frame integral of motion is derived, and this is used to show certain candidate periodic functions to be inadmissible. The system dynamics are then linearized to expose stability properties of the solutions, and it is established that asymptotic stability is impossible for all orbit families. Finally, the degree of instability in the assumed motions, over free parameter ranges, is determined numerically via the Floquet multipliers of the associated full-cycle state-transition matrices.