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.     

基于CATIA/CAA飞机蒙皮边缘连接孔最小边距快速检测方法

在新机研制阶段,设计部门提供的工程数据集可能存在连接孔边距不符合规范要求,也可能出现连接孔进入零件的R区等现象.通过对边距的检测可以检查连接孔边距的缺陷,因此边距的快速检测是一个重要问题.提出了边距提取和最小边距快速检测的算法,利用CAA/CATIA开发平台,开发了蒙皮边缘孔最小边距的快速检测软件可快速筛选不符合要求的蒙皮边缘孔并标注出来,减少了飞机生产过程中不必要的浪费,提高了生产效率.     

单孔容腔瞬态充气换热的理论分析方法

换热对于容腔瞬态响应过程有显著影响，而目前缺乏分析容腔瞬态过程换热的通用方法，导致容腔瞬态响应模拟精度较差。针对这一现状，基于自由射流、冲击射流及外掠平板换热理论，提出了一种模拟非绝热单孔容腔瞬态充气过程换热的理论方法。应用该方法模拟了容腔压力和温度的瞬态响应过程，并与试验数据进行了对比。结果表明：该理论方法的模拟结果与试验数据吻合很好，压力最大相对误差不超过3%，温度最大相对误差不超过1%，验证了理论方法的可行性和准确性。而绝热模型的模拟结果与试验数据相比，压力和温度的最大相对误差分别可达12%和14%，等温模型的压力和温度的最大相对误差分别可达6%和7%，说明理论方法显著提高了容腔瞬态响应模拟精度。同时，理论分析方法不仅具有较强的通用性，还能够极大地降低分析容腔瞬态换热的成本，可以有效支撑空气系统非绝热容腔元件建模。     

某型晶闸管恒加寿命试验中数据处理的Bayes方法

对寿命服从Weibull分布的某型晶闸管恒定应力加速寿命试验中的零失效数据,运用经典的统计方法和Bayes方法进行了处理,分别给出了在正常应力下失效概率的极大似然估计和多层Bayes估计,对2种估计结果与现场试验数据下所得估计结果的比较表明,Bayes估计的绝对误差为5.89×10-5,它小于极大似然估计的绝对误差2.438×10-3。随机模拟表明本文所给方法正确有效。     

火星探测器降落伞系统综述

文章介绍了美国火星探测器降落伞系统组成和验证试验情况;分析了5种不同探测器降落伞系统的具体差异;归纳了探测器降落伞系统的结构和性能参数;重点介绍了"凤凰号"和"火星科学实验室"降落伞系统研制过程和性能验证试验。     

电推进航天器的特殊环境及其影响

文章介绍了应用离子和霍耳电推进系统在航天器周围产生的等离子体和电磁场等特殊环境,讨论了这些特殊环境对航天器各分系统或部件产生的溅射腐蚀、沉积污染、充放电、等离子体干扰、碰撞动力学扰动等影响效应,探讨了研究电推进与航天器相互作用效应的地面试验技术、空间飞行试验技术和模型分析技术,介绍了离子电推进系统与航天器相容性分析评价的技术要点。     

卫星发动机羽流污染模型的DSMC方法研究

文章通过DSMC（Direct Simulation Monte Carlo,直接模拟蒙特卡罗）方法对卫星发动机羽流进行数值模拟,对仿真方法进行了对比验证,证实了DSMC方法可以比较精确地模拟羽流场。在建立卫星污染模型的过程中,针对污染发动机喷口形状的变化以及出口参数的变化,对DSMC方法模拟结果进行了对比,得到喷口形状和出口参数的变化对模拟结果的影响,并得到最优的卫星敏感表面羽流污染计算模型。     

空间环境研究的现状与展望

空间环境研究的内容包括空间环境模式研究、空间环境效应研究和空间环境实验研究。当前国外空间环境研究注重对大型软件组织多学科、多单位长期合作研究;模式研究与实验研究紧密结合;注意开发对工程适用的模式;工作重点是太阳帆板带电和低轨卫星表面带电。建议我国在今后的空间环境研究中加强联合,集中攻克急需的大型软件;加强对材料特性的实验研究;着手发射环境效应卫星;开拓空间环境研究的新领域;在空间环境效应研究中加强卫星研制单位、卫星操作部门与环境效应研究单位的合作。     

频率选择表面(FSS)柔性屏铺覆工艺对透波窗口透波性能的影响

为了研究工程中柔性FSS屏铺覆工艺对透波窗口通带插损的影响,设计并制备了几种不同工艺缺陷的平板,采用自由空间传输反射法研究了平板在不同入射角下的通带损耗.结果 表明:拼接缝隙使通带损耗在0°和60°入射角下增加了0.3dB;拼接褶皱使通带损耗在0°入射角下增加了0.77 dB,在60°入射角下增加了1.55 dB;多层...