嫦娥一号卫星的地月转移变轨控制

文章阐述了嫦娥一号卫星地月转移阶段(从星箭分离到进入使命轨道)的高可靠、高精度自主变轨控制方案,介绍了飞行轨道、轨控策略及控制参数优化、星上自主变轨控制的系统设计和相关参数的地面标定等,给出了在轨飞行试验的验证结果。     

天宫一号目标飞行器控制计算机的设计与验证

与载人航天一期＂轨道舱＂相比,载人航天二期天宫一号目标飞行器对控制计算机的功能、性能和环境适应性都提出了更高的要求.依据GNC分系统对控制计算机的功能与可靠度需求,介绍天宫一号目标飞行器控制计算机的容错方案、硬件设计、系统软件设计、可靠性分析和试验验证情况,地面验证结果表明：天宫一号目标飞行器控制计算机设计满足GNC分系统的需求.     

控制力矩陀螺在天宫一号目标飞行器姿态控制上的应用

根据天宫一号目标飞行器的特点及交会对接任务需求,天宫一号目标飞行器选择单框架控制力矩陀螺作为姿态控制执行机构,这是控制力矩陀螺首次在国内航天器上应用．阐述了单框架控制力矩陀螺在天宫一号目标飞行器姿态控制上的应用,主要包括四个方面：构形选择、操纵律设计、角动量卸载、故障诊断与重构．天宫一号目标飞行器控制力矩陀螺系统采用五棱锥构形,其操纵律设计为带零运动的伪逆操纵律,控制力矩陀螺系统具备故障诊断和重构功能．     

北斗星基增强系统单频服务区域可用性评估

在研究美国广域增强系统(WAAS)与欧洲地球同步导航重叠系统(EGNOS)服务可用性评估方法的基础上,基于连续8天的实测数据对当前北斗星基增强系统(BDSBAS)单频服务一类垂直引导进近(APV-I)的区域可用性进行了初步评估.评估结果表明,受系统实际播发的卫星完好性参数有效性与电离层格网点(IGP)分布的限制,中国大...     

基于L1趋势滤波的飞控传感器降噪方法

针对飞行控制传感器中普遍存在的噪声信号,提出了一种基于L1趋势滤波技术的在线降噪方法。首先简要介绍了L1趋势滤波技术,引入了滑动窗口对算法进行改进以满足实时在线应用需求。以气压计所采集的信号为例,采用原始飞参数据,利用该方法进行降噪处理,并与文献中常用的小波降噪方法进行初步比较,基于Matlab的仿真结果验证了该方法的可行性。     

压制工艺和粒径对粉末冶金Ti-1Al-8V-5Fe合金组织性能的影响

采用粉末冶金技术以氢化钛（TiH₂）粉和不同粒径的元素粉体为原料制备Ti-1Al-8V-5Fe（Ti-185）合金,研究了压制工艺对不同粒径元素粉制备的Ti-185合金组织及性能的影响。结果表明：当压制压力在800 MPa、保压时间80 s、压制速率为1 mm/s时,Ti-185生坯密度最高,为最佳压制工艺。由粒径较小元素粉制备得到的Ti-185合金晶粒越细小,合金的烧结致密度就越高。粉末粒径越小,烧结过程中合金元素实现合金化需要扩散的距离就越短,越有利于合金力学性能的提高,其中具有最小粒径的样品表现出最高的硬度（43 HRC）和强度（1 438 MPa）。     

弹载电子设备寿命预测方法研究

介绍了寿命预测的基本概念及目前较常用的几种预测方法,分析了这几种方法的优缺点。着重描述了具有"少数据建模"特点的灰色GM(1,1)预测模型的建模方法及后验差精度检验方法,最后应用此模型解决了某型号弹载电子设备寿命预测的问题。     

Cu58MnCo钎焊1Cr11Ni2W2MoV马氏体不锈钢接头组织与性能

采用Cu58MnCo钎焊连接1Cr11Ni2W2MoV,研究了工作气氛、钎焊温度和保温时间对接头组织和性能的影响。结果表明：钎焊接头主要包括α''+[γ（Fe）,γ（Mn）]相,α（Co）+δ相和[Cu,γ（Mn）]+α（Mn）相;钎焊温度升高或保温时间延长,α''+[γ（Fe）,γ（Mn）]相和[Cu,γ（Mn）]+α（Mn）相增多,α（Co）+δ相含量减少,接头拉剪强度降低;工作气氛为70 Pa时所获接头性能优于真空度1×10^－2下所得的接头性能。     

钛合金板超塑性成形/扩散连接成形因素影响的数值模拟

通过对超塑性成形与扩散连接(SPF/DB)成形原理和过程的讨论,以最优成形温度下的Ti-6AL-4V合金材料特性和超塑性成形气压加载理论优化结果为依据,利用Ansys有限元软件的建模和数值模拟,提取夹层板作为研究对象,建立模型和定义材料性能参数,定义接触和加载方式。     

A Portrait of the Nucleus of Comet 67P/Churyumov-Gerasimenko

In 2003, comet 67P/Churyumov–Gerasimenko was selected as the new target of the Rosetta mission as the most suitable alternative to the original target, comet 46P/Wirtanen, on the basis of orbital considerations even though very little was known about the physical properties of its nucleus. In a matter of a few years and based on highly focused observational campaigns as well as thorough theoretical investigations, a detailed portrait of this nucleus has been established that will serve as a baseline for planning the Rosetta operations and observations. In this review article, we present a novel method to determine the size and shape of a cometary nucleus: several visible light curves were inverted to produce a size–scale free three–dimensional shape, the size scaling being imposed by a thermal light curve. The procedure converges to two solutions which are only marginally different. The nucleus of comet 67P/Churyumov–Gerasimenko emerges as an irregular body with an effective radius (that of the sphere having the same volume) = 1.72 km and moderate axial ratios a/b = 1.26 and a/c = 1.5 to 1.6. The overall dimensions measured along the principal axis for the two solutions are 4.49–4.75 km, 3.54–3.77 km and 2.94–2.92 km. The nucleus is found to be in principal axis rotation with a period = 12.4–12.7 h. Merging all observational constraints allow us to specify two regions for the direction of the rotational axis of the nucleus: RA = 220°^+50° _−30° and Dec = −70^° ± 10^° (retrograde rotation) or RA = 40°^+50° _-30° and Dec = +70^°± 10^° (prograde), the better convergence of the various determinations presently favoring the first solution. The phase function, although constrained by only two data points, exhibits a strong opposition effect rather similar to that of comet 9P/Tempel 1. The definition of the disk–integrated albedo of an irregular body having a strong opposition effect raises problems, and the various alternatives led to a R-band geometric albedo in the range 0.045–0.060, consistent with our present knowledge of cometary nuclei. The active fraction is low, not exceeding ~ 7% at perihelion, and is probably limited to one or two active regions subjected to a strong seasonal effect, a picture coherent with the asymmetric behaviour of the coma. Our slightly downward revision of the size of the nucleus of comet 67P/Churyumov-Gerasimenko resulting from the present analysis (with the correlative increase of the albedo compared to the originally assumed value of 0.04), and our best estimate of the bulk density of 370 kg m⁻³, lead to a mass of ~ 8 × 10¹² kg which should ease the landing of Philae and insure the overall success of the Rosetta mission.