超声振动钻削装置设计与研究

为解决碳纤维复合材料和钛合金钻孔加工过程中钻头磨损严重、加工孔质量差等问题,研制了一款超声振动钻削装置.超声振动钻削装置的性能取决于声振系统设计的好坏.本文首先对声振系统的结构设计进行了理论探讨,然后采用ANSYS软件对其进行了模态分析和谐响应分析.在碳纤维复合材料和钛合金的初步钻削试验中,超声振动钻孔和普通钻孔相比轴向钻削力分别减少了48％和31％,结果表明所研制的超声振动钻削装置具有良好的钻削性能.     

用蒙特卡罗方法研究质子在航天器内部充电中的作用

介绍了航天器内部充电的基本物理机制, 重点研究了质子在内部充电中的作用. 用蒙特卡罗方法模拟质子在介质中的输运过程, 计算了简化的平板介质在一定通量的粒子环境中的内部充电情况. 结果表明, 介质内部最大电场与入射质子能量有关, 当质子能量达到14 MeV时候, 内部电场最强; 当质子与电子的入射数目相同, 并且材料参数一样时, 质子产生的最大电场大于电子产生的最大电场. 选取2004年7月26日TC-2卫星姿控分系统故障前的质子和电子通量数据, 分别计算了二者可能引起的内部最大电场. 计算结果表明,质子产生的最大电场比电子产生的最大电场小2~4个数量级, 并且远小于击穿电场; 在某些极端情况下, 例如质子产生的电场和电子产生的电场方向一致的时候, 电场的叠加会使局地电场得到加强.      

卫星用光纤陀螺三轴组合的关键技术

研究了空间环境对光纤陀螺各项指标的影响,设计了一种新颖的卫星用光纤陀螺三轴组合.针对空间辐射、温度循环和真空环境对光纤陀螺的影响进行了模拟实验,通过分析实验数据得到了空间环境对光纤陀螺主要参数的影响机理.利用最小二乘滤波的方法建立了偏置误差模型,利用查表法建立了标度因数误差模型,并用现场可编程门阵列(FPGA)实时进行零偏和标度因数补偿,补偿后陀螺输出零偏稳定性为0.1(°)/h.同时详细分析了陀螺在空间低角速度环境下产生死区的原因,并利用周期相位扰动调制的方法消除了死区.在卫星用光纤陀螺三轴组合的设计中,实现了光源复用和冗余、空间主动和被动防护措施、在轨故障诊断等技术.      

一种磁悬浮飞轮增益预调交叉反馈控制方法

磁悬浮飞轮转子在高转速下表现出的陀螺效应是影响系统稳定性的主要因素.为了提高磁悬浮飞轮的失稳转速,针对陀螺效应引起的系统章动失稳和进动失稳,提出了一种基于转速的增益预调交叉反馈控制方法,针对不同的转速段,建立在线控制相对应的交叉反馈通道增益和带宽参数表,对进动模态和章动模态分别实现交叉相位补偿.采用该控制方法用经典控制理论中的根轨迹法对系统的章动稳定性进行了仿真并对控制参数进行了优化.仿真和实验结果表明,采用这种基于转速的增益预调交叉反馈的控制算法,能够有效地抑制磁悬浮飞轮转子陀螺效应所导致的章动失稳,所设计的磁悬浮飞轮原理样机能够稳定运行在其额定转速30000r/min.      

全动复合材料水平尾翼主承力壁板热压罐成型工艺

叙述了全动复合材料水平尾翼主承力壁板热压罐成型工艺,介绍了壁板成型工艺中的关键技术,解决了壁板批量生产中提出的技术问题。     

浅谈廊坊电子信息产业的现状与发展

电子信息产业发展对当今世界经济发展起着十分重要的作用.如何加快电子信息产业发展,对保持经济持续快速增长,加快推进工业化进程具有十分重要的意义.本文立足于廊坊电子信息产业发展的现状,对未来如何加快发展廊坊电子信息产业提出自己的想法和建议.     

月球探测器动力下降段最优轨迹参数化方法

为保证月球探测器进入姿态调整段时具有充分的高度与速度余量,本文提出一种基于控制变量参数化的月球探测器动力下降段最优轨迹求解方法.在三维探测器软着陆动力学模型基础上,将月球探测器软着陆制导律设计等效为燃料最优约束下的探测器俯仰角控制问题,利用控制变量参数化(Control Variables Parameterizati...     

Design of Drilling and Riveting Multi-functional End Effector for CFRP and Aluminum Components in Robotic Aircraft Assembly

To fulfill the demands for higher quality,efficiency and flexibility in aviation industry,a multi-functional end effector is designed to automate the drilling and riveting processes in assembling carbon fiber reinforced polymer(CFRP)and aluminum components for a robotic aircraft assembly system.To meet the specific functional requirements for blind rivet installation on CFRP and aluminum materials,additional modules are incorporated on the end effector aside of the basic processing modules for drilling.And all of these processing modules allow for a onestep-drilling-countersinking process,hole inspection,automatic rivet feed,rivet geometry check,sealant application,rivet insertion and installation.Besides,to guarantee the better quality of the hole drilled and joints riveted,several online detection and adjustment measures are applied to this end effector,including the reference detection and perpendicular calibration,which could effectively ensure the positioning precision and perpendicular accuracy as demanded.Finally,the test result shows that this end effector is capable of producing each hole to a positioning precision within ±0.5 mm,aperpendicular accuracy within 0.3°,a diameter tolerance of H8,and a countersink depth tolerance of±0.01 mm.Moreover,it could drill and rivet up to three joints per minute,with acceptable shearing and tensile strength.     

Development and Prospectives of Ultra-High-Speed Grinding Technology

Ultra-high-speed grinding(UHSG)is a significant and powerful machining method in view of the enhanced productivity and precision demands.Previous researches regarding formation mechanisms and crucial technologies are comprehensively and thoroughly summarized to highlight state-of-art technology of UHSG.On the basis of the interdependence between process and machine innovations,theoretically,grinding mechanisms in strain hardening,strain rate strengthening,thermal softening,size effect and process characteristics need more in-depth studies to clarify the dominance of UHSG.Technically,CFRP wheel integrating with the brazed bonding has a prominent advantage in bonding strength and grit′s configuration over vitrified bonding,which would be superior in UHSG.Furthermore,external high pressure cooling combining with inner jet cooling methods,accompanied by scraper plates to alleviate the effect of air boundary,are crucial and practical measures for realizing effective cooling in UHSG.Grinding processes,especially those being related to grinding parameters and precise in-process measuring approaches,are also prerequisite for fitting and investigation of UHSG.     

Statistical study of energetic electrons in Jupiter’s inner magnetosphere by Juno/JEDI

The Juno spacecraft made the first in-situ observations of energetic particles in the polar region of Jupiter’s magnetosphere. After Jupiter Orbit Insertion (JOI) in July 2016, data from ~20 Juno perijoves (PJs) obtained by Juno/JEDI are accumulated, providing an excellent opportunity to study the long term spatio-temporal distribution of energetic particles in Jupiter’s radiation belt. We transform Juno’s position from a Cartesian to a magnetic coordinate system by tracing magnetic field lines based on a fourth order Runge-Kutta method. Then the fluxes of energetic electrons from PJ1 to PJ14 sorted by different locations in magnetic coordinate space and the data are well organized by the L-shell parameter. The variation of electron flux increases with L-shell. The deviation (the ratio of the 75th percentile to the 25th percentile) of 0.51 MeV electron flux varies from a factor of 1.23 near L = 9.5 to 27.57 near L = 15.5. However, the mean flux decreases by about one order of magnitude in the same region. The electron spectra at larger L-shells are softer than that at smaller L-shells. On the other hand, the electron flux decreases more rapidly with increased L-shell when the location is off the equator. Along an L-shell, the electron flux decrease at first and then increase again from equator to mid-latitude region. In addition, we compare the statistical results with the widely used GIRE2 model. JEDI data correspond well with the GIRE2 model when the L-shell is > 14.75. GIRE2 underestimate the electron flux for L-shell smaller than 13.25. These results of this analysis are applicable to estimate the effects of the radiation environment in Jupiter’s magnetosphere.