槽外聚能式超声波法清除燃油总管内腔积碳

为了克服用传统方法清除燃油总管内腔积碳的不彻底性，提出了槽外聚能式超声波清洗法。首先着重介绍了应用槽外聚能式超声波清洗技术清除发动机燃油总管内腔积碳的基本原理然后介绍了燃油总管专用超声波清洗机的开发与研制，以及超声波清洗工艺的研究过程，最终确定了槽外聚能式超声波清洗法清除燃油总管内腔积碳的清洗液配方和工艺路线。并成功应用于某大修机的生产过程。     

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.     

直升机尾桨故障及其试飞研究

介绍了直升机尾桨故障类型及其处理方法和试飞方法。探讨了发动机功率、空速、飞行高度等因素对尾故障试飞的影响。在实际试飞的基础上，给出了正确处理尾桨故障的基本方法，为直升机飞行员在飞行时遇到类似故障后的处理及有关研究人员提供了重要的参考。     

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。     

飞机主操纵系统疲劳试验载荷监控方法研究——应变数据分析法

针对某机全机主操纵系统疲劳试验中动态操纵情况下的应变测量以及试验载荷监控问题进行了分析和讨论,并对基于应变测量数据分析的操纵系统疲劳试验载荷监控方法的确定及其应用效果进行了阐述。在操纵系统疲劳试验过程中的实际监控结果表明,该方法对副翼/平尾/方向舵操纵系统多种试验状态下的试验载荷监控实用有效。     

机翼优化设计中颤振特性的快速预估方法

某民机型号研制中，为改进飞机性能对机翼部件进行了结构优化设计，而机翼的颤振特性是衡量结构优化设计方案是否满足设计要求的一项重要指标。这里介绍了一种颤振特性快速预估方法，用于研究机翼优化设计中结构刚度降低对机翼颤振特性的影响趋势。并用此方法对该飞机机翼结构优化设计方案进行了机翼翼面刚度及颤振特性预估，迅速评估了优化方案是否满足颤振设计要求。     

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.     

环境设计中的光效应与色彩

本文对光与色的关系进行了简要的阐述。从光与色的概念到对人们的心理感受，对形体的感受以及同环境的关系，可以了解到光的效应同色彩的组合参考建筑环境设计的重要性。     

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。     

上摆式客车行李舱门的设计

主要介绍了客车行李舱门的工作原理．对比了传统的与新式的行李舱门的结构，并提出了新式客车行李舱门的设计方案。根据运动要求确定出机构的主要尺寸参数，对AD杆进行受力情况分析，通过强度计算证实这种机构工作的可靠性．