产生标准失真源的方法

介绍了失真的测量原理和产生标准失真源的方法；介绍了失真度测量仪自动测试系统，并对测量装置的误差进行了分析。     

Magnetosphere Imaging Instrument (MIMI) on the Cassini Mission to Saturn/Titan

The magnetospheric imaging instrument (MIMI) is a neutral and charged particle detection system on the Cassini orbiter spacecraft designed to perform both global imaging and in-situ measurements to study the overall configuration and dynamics of Saturn’s magnetosphere and its interactions with the solar wind, Saturn’s atmosphere, Titan, and the icy satellites. The processes responsible for Saturn’s aurora will be investigated; a search will be performed for substorms at Saturn; and the origins of magnetospheric hot plasmas will be determined. Further, the Jovian magnetosphere and Io torus will be imaged during Jupiter flyby. The investigative approach is twofold. (1) Perform remote sensing of the magnetospheric energetic (E > 7 keV) ion plasmas by detecting and imaging charge-exchange neutrals, created when magnetospheric ions capture electrons from ambient neutral gas. Such escaping neutrals were detected by the Voyager l spacecraft outside Saturn’s magnetosphere and can be used like photons to form images of the emitting regions, as has been demonstrated at Earth. (2) Determine through in-situ measurements the 3-D particle distribution functions including ion composition and charge states (E > 3 keV/e). The combination of in-situ measurements with global images, together with analysis and interpretation techniques that include direct “forward modeling’’ and deconvolution by tomography, is expected to yield a global assessment of magnetospheric structure and dynamics, including (a) magnetospheric ring currents and hot plasma populations, (b) magnetic field distortions, (c) electric field configuration, (d) particle injection boundaries associated with magnetic storms and substorms, and (e) the connection of the magnetosphere to ionospheric altitudes. Titan and its torus will stand out in energetic neutral images throughout the Cassini orbit, and thus serve as a continuous remote probe of ion flux variations near 20R _S (e.g., magnetopause crossings and substorm plasma injections). The Titan exosphere and its cometary interaction with magnetospheric plasmas will be imaged in detail on each flyby. The three principal sensors of MIMI consists of an ion and neutral camera (INCA), a charge–energy–mass-spectrometer (CHEMS) essentially identical to our instrument flown on the ISTP/Geotail spacecraft, and the low energy magnetospheric measurements system (LEMMS), an advanced design of one of our sensors flown on the Galileo spacecraft. The INCA head is a large geometry factor (G ∼ 2.4 cm² sr) foil time-of-flight (TOF) camera that separately registers the incident direction of either energetic neutral atoms (ENA) or ion species (≥5^∘ full width half maximum) over the range 7 keV/nuc < E < 3 MeV/nuc. CHEMS uses electrostatic deflection, TOF, and energy measurement to determine ion energy, charge state, mass, and 3-D anisotropy in the range 3 ≤ E ≤ 220 keV/e with good (∼0.05 cm² sr) sensitivity. LEMMS is a two-ended telescope that measures ions in the range 0.03 ≤ E ≤ 18 MeV and electrons 0.015 ≤ E≤ 0.884 MeV in the forward direction (G ∼ 0.02 cm² sr), while high energy electrons (0.1–5 MeV) and ions (1.6–160 MeV) are measured from the back direction (G ∼ 0.4 cm² sr). The latter are relevant to inner magnetosphere studies of diffusion processes and satellite microsignatures as well as cosmic ray albedo neutron decay (CRAND). Our analyses of Voyager energetic neutral particle and Lyman-α measurements show that INCA will provide statistically significant global magnetospheric images from a distance of ∼60 R _S every 2–3 h (every ∼10 min from ∼20 R _S). Moreover, during Titan flybys, INCA will provide images of the interaction of the Titan exosphere with the Saturn magnetosphere every 1.5 min. Time resolution for charged particle measurements can be < 0.1 s, which is more than adequate for microsignature studies. Data obtained during Venus-2 flyby and Earth swingby in June and August 1999, respectively, and Jupiter flyby in December 2000 to January 2001 show that the instrument is performing well, has made important and heretofore unobtainable measurements in interplanetary space at Jupiter, and will likely obtain high-quality data throughout each orbit of the Cassini mission at Saturn. Sample data from each of the three sensors during the August 18 Earth swingby are shown, including the first ENA image of part of the ring current obtained by an instrument specifically designed for this purpose. Similarily, measurements in cis-Jovian space include the first detailed charge state determination of Iogenic ions and several ENA images of that planet’s magnetosphere.This revised version was published online in July 2005 with a corrected cover date.     

基于VXI总线的检测软件设计

基于VXI总线和虚拟仪器技术，研制开发了用于外场的模拟式电子控制器检测软件，并对软件开发的过程和要求进行了分析，重点解决了程序设计中的需求分析和模块化设计问题。     

具有自学习功能的机载火控系统故障诊断系统研究

研究了一种应用于机载火控系统的具有自学习功能的故障诊断系统.首先介绍了系统的总体结构;然后通过分析火控系统的结构建立了层次诊断模型,并通过示例对诊断系统中知识的表达方法、推理方法等问题做了详细的分析;最后详细描述了系统的自学习机制.应用具有自学习功能的故障诊断专家系统,可实现综合化机载火控系统的智能故障诊断.     

稳态周向混合畸变对压气机特性和流场的影响

用完全径向平衡方程加多扇平行压气机模型处理复杂畸变流场的方法，计算出进口流场组合参数畸变对压气机特性和性能的影响，并得出了压气机在进口畸变条件下流场的详细情况。     

超燃冲压发动机隔离段流场数值模拟

隔离段是双模态超燃冲压发动机实现双模态和模态转换的一个重要部件,同时,它把进气道和燃烧室隔离开,以防止燃烧室工作对进气道干扰,引起进气道不启动。由于隔离段内气体流动的复杂性及其广泛的工程应用前景,隔离段内的流动特性引起了人们的广泛关注。本文使用隐式TVD格式,采用雷诺应力湍流模型,近壁面采用非平衡壁面函数方法处理,控制方程的离散采用二阶迎风格式,对隔离段内的流场进行了数值模拟,并分析了出口反压、来流马赫数对隔离段内流场的影响。     

GH4169合金疲劳裂纹扩展性能的试验研究

本研究中对GH4169高温合金的疲劳裂纹扩展性能进行了试验研究。主要进行了400℃～600℃范围内的疲劳裂纹扩展试验．其中对GH4169环形锻件进行了室温下的疲劳裂纹扩展试验。结果表明，在400℃-600℃范围内，温度对GH4169高温合金疲劳裂纹扩展性能的影响很小，随温度上升，裂纹扩展速率稍有加快；优质成分对GH4169高温合金的疲劳裂纹扩展性能几乎没有影响，在相同温度下，YZGH4169与GH4169的疲劳裂纹扩展速率几乎一样；材料品种对YSGH4169高温合金的疲劳裂纹扩展性能有一定影响，YSGH4169锻件比棒材的疲劳裂纹扩展性能要好一些。     

快速凝固Al88Ce2Ni7Fe3非晶铝合金初生型晶化的研究

用X光衍射和透射电镜研究证实快速凝固Al88sCe2Ni7Fe3非晶铝合金晶化过程中的初期阶段为初生型晶化。初生相α－Al的结晶体积分数和纳米晶体尺寸随退火温度的升高表现出非同步增长行为：前者逐渐增加而后者变化不明显。不同退火态样品的小角X光散射结果表明，非晶基体中不断析出的纳米晶α－Al粒子，由开始的低温稀疏分布转向高温密集分布。根据实验结果，分析和讨论初生相α－Al的体积分数、晶粒数目、粒子尺寸及粒子分布在初生型晶化过程中的变化规律，为纳米晶α－Al粒子强化非晶基体提供了清晰的物理图像。     

关于确立CAD软件绘制标准化工程图地位的探讨

工程图样作为工程技术信息交流的必要手段,在工程设计与制造中起到举足轻重的作用,而繁琐的手工绘图又一直困扰着工程技术人员,计算机辅助绘图为解决这一问题提供了有利手段。但是工程图样既然作为交流文件,它的图形、标记以及表达形式都要严格执行《机械制图国家标准》。而目前ＣＡＤ绘图软件中普遍缺少处理机械图样标准化功能的现象,必然要直接影响绘制工程图的质量和速度。本文的目的在于研究ＣＡＤ软件的绘图功能与我国工程     

飞机概念设计中的生存力效益/代价综合评估方法

 首先介绍了军用飞机在常规武器威胁下的生存力评估指标及几种提高生存力措施；其次研究了将全因素试验法应用于评价生存力提高措施对生存力评估指标的增益影响的可行性；最后基于飞机的安全性、维修性、可靠性、保障性、性能及费用等约束条件，建立了一种能应用全因素试验法在飞机概念设计中进行飞机生存力效益／代价综合评估的方法。算例初步说明了方法的有效性。