直角切削6061-T6铝合金剪切区力学行为及微观结构演化预测

力学行为是塑性变形微观过程的宏观表现,早期的金属切削理论模型没有考虑微观结构对切削力的影响。在考虑热力耦合效应的基础上建立了基于位错密度材料模型的6061-T6铝合金直角切削力预测模型,分析了不同切削参数下基于位错运动的塑性变形机制对切削力的影响。结合等分剪切区和非等分剪切区模型,构建了第一变形区多物理场计算方法,提出一种切屑形成过程中由塑性变形引起的微观结构演化解析模型。通过测量切削力和切屑内晶粒尺寸对模型的可行性进行了初步验证。结果表明：剪切区长度变长引起参与位错滑移的材料增多是切削深度增大导致切削力增大的主要原因。增大切削速度导致切削力的降低不是单一变量影响的结果,而是应变降低引起位错增殖数量减少和温度升高引起位错湮灭作用增加的共同作用结果。非等分剪切区模型正确反映了第一变形区温度和应力的分布特征,且与二维有限元模型分布相一致,建立的第一变形区微观结构演化解析模型能够预测切屑内位错密度和晶粒尺寸。     

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。     

关于电磁频谱作战的思考

电磁频谱作战能力是打赢未来体系化战争的必要能力,是实现战争信息化与智能化的核心基础。随着作战域维度的不断增加,通过掌控电磁频谱以获得战场信息主动权,实现跨作战域高维度的协同与融合是掌控战争的终极制胜目标。通过回顾电磁域对抗演变的全过程,分析掌控电磁频谱能力的必要性,并从低-零功率电磁频谱战、电磁机动作战、制电磁权与制信息权、电子对抗系统技术等方面阐述电磁频谱作战所面临的挑战与发展需求,最后在组织管理、理论研究、关键技术、评估验证等方面提出加强电磁频谱作战能力的发展建议。     

星载某设备高阻接地设计对整星电磁兼容性的影响

为了满足新的使用需求,星载某设备的接地设计由壳体直接接地改为采用高阻接地。文章采用理论分析和软件仿真的方法,对该设备采用高阻接地的设计后对整星电磁兼容性能的影响进行了分析,并提出了专项试验验证方法,在故障模拟仿真卫星平台上实施了试验验证。仿真分析和试验验证都表明,此设备采用高阻接地的设计不会对卫星整星的电磁兼容性产生明显影响,可作为后续其他卫星型号采用此类设计的参考。     

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.     

霍尔推力器羽流对S波段电磁波的衰减研究

霍尔推力器羽流对S波段电磁波信号有衰减作用,这对星上推力器与天线的布置策略有重要影响。为研究S波段电磁波的衰减程度,建立几何光路算法,对电磁波在等离子体羽流媒质中的传输衰减进行数值描述,并以试验所测的信噪比数据来验证算法精度。验证试验采用空间透射波法,在相同工况的试验与计算结果对比中,最大计算误差为26.1%,平均误差为7.3%;在趋势上,试验结果与计算结果保持一致。在此基础上,针对84个在轨典型工况进行S波段电磁波信噪比衰减计算,结果显示：羽流对电磁波的吸收作用是影响衰减的主要因素,衰减最大区域出现在天线位置0.3～0.6m、方向角15°～30°的区域,衰减值在-7~-4dB之间。该结果可为霍尔推力器与天线在卫星的布置提供参考依据。