钛合金螺旋铣孔孔径偏差研究

螺旋铣孔是航空航天领域新出现的制孔技术,其切削过程中会产生径向切削力,从而引起刀具变形并造成孔径偏差。针对该问题开展了钛合金螺旋铣孔孔径偏差试验,分析了包括进给方向在内的不同加工参数对孔径偏差的影响规律;基于螺旋铣孔运动学原理对不同进给方向下的材料去除过程和径向切削力方向进行了研究,分析了不同进给方向下的孔径偏差变化规律及形成原因,并设计切削力试验进行了验证;通过分析不同加工参数下的未变形切屑形状及径向切削力变化情况,研究了各加工参数对孔径变化趋势的影响规律。研究结果表明,当进给方向为顺时针时,刀具受背离孔心的径向切削力的作用向孔径外侧发生挠曲变形,导致所加工孔径大于理论孔径;当进给方向为逆时针时则相反。进给速度和导程的增加将加剧孔径偏差,切削速度的增加则会减弱孔径偏差。     

Approach to Interference Riveting Process Control of Aircraft Automatic Drilling and Riveting

Interference fit riveting is an effective way to improve the fatigue life of aircraft.The accurate control of riveting interference of aircraft automatic drilling and riveting equipment is achieved by process parameters including upsetting force and upset head height.It is valuable for aircraft manufacturing engineering.An approach to interference riveting process control based on the analysis of interference riveting stress field is proposed.According to assembly structure,the upsetting force is calculated by the material property and interference fit level,and the upset head height is deduced by the upsetting force.The experimental result shows that the interference fit level can be controlled accurately by the upsetting force and upset head height,and then,the quality of aircraft automatic riveting can be improved.The proposed approach is verified by the good match between the predicted result and the experimental result.     

CFRP曲面铣削力及加工缺陷研究

碳纤维增强复合材料(Carbon fiber reinforced polymer,CFRP)曲面结构不断变化的工件倾角使得在加工过程中易产生分层、毛刺等缺陷。为研究工件倾角对CFRP曲面结构可加工性的影响规律,采用金刚石涂层铣刀对不同倾角下CFRP叠层平板结构进行顺铣加工试验,对不同坐标系下的铣削力和加工侧面、表面缺陷进行了研究。研究结果表明,随工件倾角的增大,水平方向上每齿所切材料平均厚度与截面积均减小,等效轴向切深逐渐增大,但是每齿去除材料体积保持不变。机床坐标系下的铣削力几乎不随工件倾角的变化而变化。而在工件坐标系下,铣削力沿工件厚度方向逐渐增大,沿工件长度方向逐渐减小。同时随着工件倾角的增大,侧面表层分层缺陷不断加重,纤维束发生弯曲,裂纹沿纤维方向逐渐扩展至表层内部,加工表面遭受破坏铺层数量也同样增加。     

有翼再入飞行器的超/高超声速气动力工程方法

有翼再入飞行器气动力的工程计算方法尚有待进一步完善,计算精度有待进一步提高。文章根据有翼再入飞行器的气动布局特点,改进和发展了一套适于其气动布局的部件划分策略和压强计算选取准则。以此对航天飞机轨道器和类X-34飞行器的纵向气动力特性进行工程计算,并与其风洞试验和数值模拟结果进行对比分析。结果表明,文中的工程计算方法在马赫数3以上的超/高超声速范围内可准确预测有翼再入飞行器的升阻特性,其中升力系数和阻力系数误差小于10%;并可准确预测俯仰力矩特性随迎角改变的变化规律。与现有方法相比,文中的部件划分策略和压强计算选取准则在升阻特性精度相当情况下,可明显提高俯仰力矩的预测精度,并反映飞行器表面的压强分布特征。     

基于自适应迭代的机器人曲面恒力跟踪

针对利用机器人进行打磨、抛光、去毛刺等场合时末端执行器对曲面工件轮廓跟踪时难以得到恒定接触力的问题,对机器人末端执行器和工件轮廓接触时的接触力进行研究,建立了实际跟踪过程中机器人末端执行器的接触力和已知传感器坐标系的映射关系,提出了一种基于自适应迭代学习算法的机器人力/位混合曲面恒力跟踪控制方法。该方法由两部分组成:基于机器人和环境接触时的阻抗模型设计了迭代学习控制律,在PD反馈控制的基础上通过迭代项克服机器人的未知参数和不确定性,并构建Lyapunov能量函数证明所提控制律的收敛性;将迭代学习控制律和力/位混合曲面恒力跟踪控制方法结合起来设计了用于曲面工件轮廓跟踪的控制方法。实验结果显示,经过15次迭代,接触力的波动范围逐渐变小并稳定在±3 N之内,验证了所提方法的有效性。      

GRACE accelerometer calibration by high precision non-gravitational force modeling

The precise modeling and knowledge of non-gravitational forces acting on satellites is of big interest to many scientific tasks and missions. Since 2002, the twin GRACE satellites have measured these forces in a low Earth orbit with highly precise accelerometers, for about 15?years. Besides the significance for the GRACE mission, these measurement data allow the evaluation of modeling approaches and the improvement of force models. Unfortunately, before any scientific usage, the accelerometer measurements need to be calibrated, namely scale factor and bias have to be regularly estimated.In this study we demonstrate an accelerometer calibration approach, solely based on high precision non-gravitational force modeling without any use of empirically or stochastically estimated parameters, using our in-house developed satellite simulation tool XHPS. The aim of this work is twofold, first we use the accelerometer data and the residuals resulting from the calibration to quantitatively analyze and validate different non-gravitational force model approaches. In a second step, we compare the calibration results to three different calibration methods from different authors, based on gravity field recovery, GPS-based precise orbit determination, and based on modeled accelerations.We consider atmospheric drag forces and winds, as well as radiation forces due to solar radiation pressure, albedo, Earth infrared and thermal radiation (TRP) of the satellite itself. For TRP, we investigate different transient temperature calculation approaches for the satellite surfaces with absorbed power from the aforementioned radiation sources. A detailed finite element model of the satellite is utilized for every force, considering orientation, material properties and shadowing conditions for each element.For cross-track and radial direction, which are mainly affected by the radiative forces, our calibration residuals are quite small when drag is not super dominant (1–3?$\text{nm}/{\text{s}}^2$ for total accelerations around $\pm$50?$\text{nm}/{\text{s}}^2$). For these directions the calibration seems to perform better than the other compared methods, where some bigger differences were found. For the drag dominated along-track direction it is vice versa, here our method is not sensitive enough because the difference between modeled and measured drag is bigger (e.g. residuals around 10?$\text{nm}/{\text{s}}^2$ for total accelerations around $\pm$70?$\text{nm}/{\text{s}}^2$ for low solar activity). In along-track direction the orbit determination based methods are more sensitive and produce more reliable results. Results for the complete GRACE mission time span from 2003 to 2017 are shown, covering different seasonal environmental conditions.     

脉冲推力轨道拦截可达性描述及求解方法

针对航天器单脉冲轨道拦截可达性分析问题,基于共面变轨、逆轨拦截假设,考虑能量、时间和交会角约束,提出了拦截航天器可拦截区和可发射区的概念。在航天器单脉冲空间可达范围的基础上,进一步考虑了目标轨道的约束,建立了目标轨道命中区的计算策略,对异面轨道交叉点为燃料最省点做出了解释。把拦截可达性相关的问题归纳为8个基本拦截问题,通过这8个问题的组合,描述了考虑能量、时间和交会角约束下拦截问题的可拦截区和可发射区的计算方法。采用圆轨道共面变轨、逆轨拦截场景进行了仿真验证,结果表明该方法能够快速有效地计算出约束条件下航天器的拦截可达范围,能够用于分析特定任务情况下的拦截可达性。     

流体的压强梯度是决定升力的重要因素

认为经典升力理论遗漏了一个决定升力的重要因素：流体的压强梯度。指出：地球上的流体都具有压强梯度,这是由地球引力引起的流体的一种不均匀性,这种不均匀性会在流体的运动中表现出来。运用“升腾效应”和“擅升效应”解释了一些与升力有关的现象,特别是解释了机翼的展弦比、机翼的厚度、雷诺数等对升力的影响,并设计了几个检验这两个效应的试验方法。     

自由分子流微电热推力器工作特性和性能研究

微推进地面试验系统由推进剂贮存供应控制单元、电源供应控制单元、虚拟仪器测控单元和推力器等组成。通过FMMFL的设计加工和地面试验系统建设,在大气状态下,对FMMR的工作特性和性能进行研究,并与理论分析和数值模拟计算结果进行了对比分析。研究结果表明,在大气状态下,基于MEMS的薄膜温度传感器和薄膜加热器工作稳定;当输入功率为14．6W,工作压强为100Pa时,推力器工作温度为600K。推进剂工质为N2时,质量流量为3．720mg／s,比冲为54．254s,推力为1．979mN;推进剂工质为H2O时,质量流量为2．976mg／s,比冲为68．163s,推力为2．000mN。FMMR的各项性能参数与理论分析结果一致。通过优化设计和系统集成,FMMR的性能将得到进一步提高。     

共位衍射电磁航天器成像过程中的小推力控制 (新型推进系统控制专栏)

为了满足衍射成像系统在解决低轨遥感航天器覆盖范围小、目标重访周期长等问题的同时,而引入的航天器相对位置、姿态控制需求。针对共位衍射航天器相对位置、姿态控制过程中传统推力器带来的羽流污染问题,本文采用电磁推力器和飞轮作为执行器,设计一种基于快速非奇异滑模的轨道控制器和基于PID的姿态控制器。所设计的快速非奇异滑模轨道控制器为共位衍射航天器频繁位置调整提供控制保障,基于PID的姿态控制器能够消除由电磁力耦合产生的电磁干扰力矩。研究结果表明：基于相对轨道动力学方程设计的快速非奇异滑模控制律鲁棒性好、收敛速度快,能够达到两颗共位衍射电磁航天器沿z轴保持在10m相对距离的控制效果。在轨道调整过程中,其姿态能够通过PID算法稳定控制到期望姿态,使衍射成像结构一直保持不变,从而有效完成衍射成像任务。