对接动力学仿真试验台再现频率指标验证

为验证对接动力学仿真试验台再现对接动力学过程中频率0~6 Hz相对运动的能力,用弹性棒方案再现频率0~6 Hz的碰撞过程,由建模与设计计算选定弹性棒的悬臂长度、刚度和航天器质量等设计参数,仿真分析了碰撞过程的接触碰撞力、变形量与速度,以及再现频率等的影响。结果表明:设计参数合理,精度考核方案可行。     

焊锡对热电偶测温误差影响分析

航天器真空热试验中为了消除焊锡可能带来的温差热电势,文章采用Keithley 2750数据测量系统,通过比较法对焊锡与铜、焊锡与康铜之间的温差热电势进行了测试分析。标准热电偶选择铜-康铜热电偶,测试温度范围为-195～+75℃。测试时,热电偶冷端为冰水混合物,热端为液氮浸泡过的不锈钢圆柱体或热水瓶。为了确保回路中的焊点处于相同的热环境条件,可采用多层隔热组件进行包覆,避免接插件直接接触热沉。     

直升机空中回收和投放货物技术发展综述

针对直升机空中回收和投放货物技术的发展进行了探讨.首先按照直升机空中回收系统发展的三个阶段,简要介绍了三代系统的特点、工作过程及典型应用实例；其次对无人直升机投放技术进行研究综述,介绍了美国K - Max直升机实现无人货运投放的技术及其应用.     

Study of riblet drag reduction for an infinite span wing with different sweep angles

This paper studies the riblet drag reduction effect for an infinite swept wing under a low Reynolds number using a large-eddy simulation. The results show that the drag reduction ratio is not linear under different sweep angles. The maximum drag reduction ratio in this study is 9.5% for a wing with a 45° sweep angle. The local surface streamline angle and turbulence quantities are calculated to analyze the drag reduction mechanism. The results demonstrate that the riblets considerably suppress the Reynolds stresses above the wing upper surface, while the turbulence kinetic energy in the near wake is increased. A possible relaminarization phenomenon is observed at the middle part of the wing. Quasi-two-dimensional flow structures are observed near the wall, and a peak frequency is considered as the dominant frequency of the region.     

黏附激励下空间目标惯性参数的辨识方法

针对黏附卫星会自然激励目标改变运动状态的现象，提出一种利用黏附激励进行空间非合作目标惯性参数的辨识方法。黏附前，利用主星对目标特征点的视觉测量，建立估计目标惯性参数与相对运动参数的滤波器，并估计目标的转动惯量比和质心；黏附后，主星直接利用该滤波器估计目标的新的质心速度，并基于动量守恒原理计算目标质量。该方法不仅充分利用黏附过程的自然激励，无需常规辨识必须的主动激励，而且激励前后算法一致，无需切换。数字仿真证实了算法的有效性。     

运载器着陆装置展开动力学及影响因素分析

以垂直起降重复使用运载器收放、锁定、缓冲一体化着陆装置及其气压驱动控制系统为研究对象,首先分析了着陆装置展开机构的运动奇异性,在此基础上,建立了展开机构动力学模型与气压驱动系统集中参数模型,将两模型相耦合从而构建了展开系统协同仿真分析模型,随后重点研究了运载器主体自旋角速度、垂向返回速度、减压阀调节压力以及支柱摩擦力对展开性能的影响。研究结果表明:运载器自旋角速度越大,产生的离心力越高,将导致支柱展开时间及各腔压力峰值减小;垂向着陆速度越高,引起的支柱气动阻力越大,将会大幅延长展开时间;减压阀调节压力的增加将缩短展开时间,但会引起各腔峰值压力上升;支柱摩擦力的增加将增大展开时间,但会减小锁定到位时间。     

Sailing with solar and planetary radiation pressure

Literature on solar sailing has thus far mostly considered solar radiation pressure (SRP) as the only contribution to sail force. However, considering a sail in a planetary mission scenario, a new contribution can be added. Since the planet itself emits radiation, this generates a radial planetary radiation pressure (PRP) that is also exerted on the sail. Hence, this work studies the combined effects of both SRP and PRP on a sail for two case studies, i.e. Earth and Venus. In proximity of the Earth, the effect of PRP can be significant under specific conditions. Around Venus, instead, PRP is by far the dominating contribution. These combined effects have been studied for single- and double-sided reflective coating and including eclipse. Results show potential increase in the net acceleration and a change in the optimal attitude to maximise the acceleration in a given direction. Moreover, an increasing semi-major axis manoeuvre is shown with and without PRP, to quantify the difference on a real-case scenario.     

Analysis of the solar sail deformation based on the point cloud method

The deformation of the solar-sail membrane is an important factor for causing inaccuracies in the solar-sail missions. This paper describes the solar sail under deformation by using a new modelling technique based on point cloud and triangular mesh generation. Two types of deformation, stemming from wrinkling and billowing, are modelled. The changes in the solar radiation pressure force and the moment caused by deformation are calculated and compared to the ideal non-deformed case. The heliocentric spiral trajectory and the orbital angular momentum reversal trajectory are taken as examples to quantify the influence of the deformation from an orbit point of view. Additionally, point cloud simplification, based on the normal vector and bounding box, is utilized to simplify the original deformed-sail model. It involves a reasonable reduction and renewal of the points in the model considering the variation of surface curvature. The simplification and its modelling accuracy are numerically investigated as well as computational efficiency.     

MSCSG随机误差测试及误差源分析

针对磁悬浮控制敏感陀螺(MSCSG)的角速率测量信号中存在较大的随机误差，不利于提高MSCSG敏感精度，以MSCSG原理样机为研究对象，提出采用Allan方差分析法对MSCSG实测数据进行随机误差分析。首先，根据MSCSG角速率敏感原理推导出MSCSG转子偏转角速率的量测公式；其次，应用Allan方差分析法和最小二乘拟合方法计算出5种典型随机误差系数。计算结果显示:在MSCSG随机误差中，零偏不稳定性、速率随机游走以及速率斜坡占主要成分，而量化噪声和角度随机游走误差所占比重较小。依此，对MSCSG误差来源进行了指向性分析，并给出了随机误差的抑制补偿方法，为MSCSG敏感精度的提高奠定了理论基础。      

Simulation of unsteady combustion in a LOX-GH2 fueled rocket engine

This paper presents results from an investigation of unsteady combustion inside a small-scale, multi-injector liquid rocket engine. A time-accurate approach in an axisymmetric geometry is employed to capture the unsteady flow features, as well as the unsteady heat transfer to the walls of the combustion chamber. Both thermally perfect gas (TPG) and real gas (RG) formulations are evaluated for this LOX-GH₂ system. The Peng–Robinson cubic equation of state (EoS) is used to account for real gas effects associated with the injection of oxygen. Realistic transport properties are computed but simplified chemistry is used in order to achieve a reasonable turnaround time. Results show the importance of the unsteady dynamics of the flow, especially the interaction between the different injectors. The RG EoS, despite a limited zone of influence, is shown to govern the overall chamber behavior. The sensitivity of the results to changes in the system parameters is studied and some general trends are discussed. Although several features of the simulations agree well with past experimental observations, prediction of heat flux using a simplified flux boundary condition is not completely satisfactory. Reasons for this discrepancy are discussed in the context of the current axisymmetric approach.