表面粗糙度的现状及发展

讨论了表面粗糙度测量和表征中,一些人们感兴趣的有待解决的问题,如：基准、滤波、校准样块、评定软件和表征参数等．认为在3D表面分析中应采用数字滤波,以保留数据的完整性;辨析了现存测量仪器和方法的范围──分辨力空间图中的缺口;介绍了校准样块的制备和测量;同时指出当前评定软件缺乏一致性和标准性,建议设计“软件量规”．最后指出了表面特征分析的发展趋势．     

Ti2SnC的合成及其反应机制的研究

采用常压烧结技术,分别对Ti/Sn/C和Ti/Sn/TiC两种配料,在950～1250℃温度范围、保温15～360 min,真空条件下进行烧结.结果表明,两种配料均在1200℃短时间内合成了高纯度Ti2SnC粉.利用X射线衍射(XRD),能量色散谱仪(EDS)及扫描电镜(SEM)对Ti2SnC粉末进行了表征,并对Ti2SnC的形成机制进行了分析.所制备的Ti2SnC为片状颗粒,表面光滑,颗粒尺寸小于10 μm,厚度约为1～2 μm.Ti2SnC的形成机制是,在Ti-Sn-C反应系统中,Ti和Sn先反应形成Ti-Sn化合物;然后是Ti和C反应形成TiC;最后,Ti-Sn化合物和TiC反应形成Ti2SnC.此反应机制进一步由Ti-Sn-TiC反应系统验证.     

高超声速一体化飞行器冷流状态气动特性研究

采用数值模拟和风洞实验方法,对高超声速一体化飞行器缩比模型在发动机关闭以及发动机通流状态下的气动特性进行研究。实验中采用彩色纹影系统对缩比模型飞行器的超声速流场进行显示,并通过六分量应力天平测得了全机的升力、阻力和俯仰力矩,数值模拟气动力系数以及流场特征与实验结果吻合较好,同时分析了飞行器保持静稳定状态下的质心选择范围。结果表明进气道开启之后飞行器升力阻力以及抬头力矩显著下降,但此飞行器配平迎角仍较大。该实验结果验证了数值方法的可靠性并为飞行器构型设计提供了参考数据。     

固体发动机老化过程中材料缺陷无损检测方式

综述了无损检测固体发动机的研究现状及应用前景，并对现有的无损检测固体发动机方法，提出了技术改进的措施。     

飞行器服役（作战）完整性的提出与发展

飞行器服役完整性（对于军用飞行器也称为作战完整性）更综合地表征了飞行器在服役（作战）使用过程中的质量特性。本文首先介绍了飞行器服役（作战）完整性概念的提出过程,讨论了飞行器服役（作战）完整性的基本内涵和基本特性,阐明了飞行器服役（作战）完整性是飞行器服役（作战）适用性与飞行器服役（作战）效能发挥的基础。然后介绍了飞行器服役（作战）完整性的三种表征参数：飞行器固有完好率、飞行器固有健康度、飞行器服役（作战）完整度,并梳理了飞行器服役（作战）完整性优化设计的基本方法。最后提出了飞行器服役（作战）完整性的控制原理,指出了飞行器服役（作战）完整性发展的基础、研究方法和目前我国航空航天领域急需研究和发展的方向。     

Surface morphology characterization of unidirectional carbon fibre reinforced plastic machined by peripheral milling

This paper aims to characterise surface morphology and 3D roughness parameters of unidirectional carbon fibre reinforced plastic（UD-CFRP） milled at 0°, 45°, 90°, and 135° fibre orientation angles（FOAs）. Side milling experiments are conducted on UD-CFRP laminates. Surface damage forms and texture direction of milled surface are analysed. Spatial frequency of defects on CFRP surface is quantitatively determined using radially averaged 2D PSD. The kinematicdynamic surface topography is reconstructe...     

芳氧基聚磷腈绝热包覆材料的性能表征

针对固体火箭发动机对绝热包覆材料性能要求,制备了芳氧基聚磷腈绝热包覆材料。利用热导率测定仪、动态热机械仪、SEM以及国军标规定的测试方法对芳氧基聚磷腈的热导率、线膨胀系数、烧蚀后碳层结构、密度、线烧蚀率以及与推进剂的相容性等进行了表征。结果表明,芳氧基聚磷腈的热导率为0.187 W/(m·K)、线膨胀系数为2.31×10-4、密度为1.196 g/cm3、线烧蚀率为0.109 mm/s,而且烧蚀后成碳率高、碳层坚硬,同时该材料与推进剂具有良好的相容性。芳氧基聚磷腈优异的物理性能及抗烧蚀性能,证明其可作为火箭发动机绝热包覆材料,并显示出良好的应用前景。     

Reconciling space object observed and solar pressure albedo-areas via astrometric and photometric data fusion

There are many Resident Space Objects (RSOs) in the Geostationary Earth Orbit (GEO) regime, both operational and debris. The primary non-gravitational force acting on these RSOs is Solar Radiation Pressure (SRP), which is sensitive to the RSO’s area-to-mass ratio. Sparse observation data and mismodeling of non-gravitational forces has constrained the state of practice in tracking and characterizing RSOs. Accurate identification, characterization, tracking, and motion prediction of RSOs is a high priority research issue as it shall aid in assessing collision probabilities in the GEO regime, and orbital safety writ large. Previous work in characterizing RSOs has taken a preliminary step in exploiting fused astrometric and photometric data to estimate the RSO mass, shape, attitude, and size. This works, in theory, since angles data are sensitive to SRP albedo-area-to-mass ratio, and photometric data are sensitive to shape, attitude, and observed albedo-area. By fusing these two data types, mass and albedo-area both become observable parameters and can be estimated as independent quantities. However, previous work in mass and albedo-area estimation has not quantified and assessed the fundamental physical link between SRP albedo-area and observed albedo-area. The observed albedo-area is always a function of the SRP albedo-area along the line of sight of the observer. This is the physical relationship that this current research exploits. It is shown through simulation that due to this physical link, and through the fusion of astrometric and photometric data, it is possible to observe the mass of a space object when the area is not known. Results for data from 100 trajectories generated from randomly sampled initial conditions are shown. It is seen that even when the area of the object is not known, the uncertainty in mass can be lowered from an initial value of 800?kg to the range 500–700?kg for 72% of the samples, 200–500?kg for 13% of the samples, and 0–200?kg for 15% of the samples. It is further shown that although the uncertainties are large, the actual errors in mass are much lower, with the error RMS being less than 100?kg for 30% of the samples, between 100 and 200?kg for another 30%, and between 200 and 300?kg for 24% of the samples.     

X 射线照相缺陷定位方法分析与验证

相对于公式法,双标记法解决了焦距和焦点位移测量误差所带来的问题.但此方法在射线检测领域普及程度并不高,其中原因,首先是原理较复杂,针对性研究少,其次是测量精度没有被量化,可信度不高.本文从公式法入手,通过对原理公式的变化分析和线性化分析,明晰了双标记法缺陷深度定位原理,推导了缺陷深度定位公式,利用简化模型,对双标记法的定位精度做了进一步的分析与计算,最后针对具体被检测物,测试验证了双标记法的计算公式和测量精度,用理论和实践证明了方法和精度的可靠性.     

质子和电子对光学反射镜辐射效应的研究

研究了能量为E=160keV质子和电子单独及综合辐照作用对两种空间反射镜光学表面的影响。观察到在辐照剂量达到Φ=10×105/cm2后反射镜表面形咸了明显的结构缺陷,并导致某些谱段反射率的降低和成像质量的下降。辐照诱发缺陷的类型及分布特征除与粒子种类和反射镜结构有关外,还依赖于试样的接地方式。质子幅照主要引起反射镜表面膜层的起泡现象;电子辐照则使SiO2保护膜着色;综合辐照的影响复杂,尤其是在接近于空间使用条件的第二种接地方式下,起泡现象和静电效应成为镜面损伤的主要机制。