固体发动机推力随机调节的涡流阀方案研究

介绍了一种固体发动机推力大小随机调节实现的方案－涡流阀方案，导出了涡流阀调节性能的相似准则方程；对涡流阀调节固体发动机静态特性和影响调节性能的各种主要因素进行了分析，指出了提出调节性能的途径，诸了模型发动机的推力调节。     

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.     

基于牛顿欧拉法的3-RPS并联机构逆动力学分析

 以3-RPS机构为例，研究了对称少自由度并联机构的逆动力学问题。因其自由度数目小于6，该类机构的支链不仅传递驱动力，同时还需为动平台提供约束。然而，现有文献大多未对广义约束力给予足够的重视。采用牛顿欧拉法建立了3-RPS机构的刚体动力学方程，给定动平台的运动规律及外载荷后，可一并求解机构所需的驱动力与约束力矩。算例仿真表明，与动平台自由速度方向不一致的外载荷主要需由约束力矩平衡。因此，在对称少自由度并联机构动力学设计中，必须计入广义约束力的影响。     

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。     

某型飞机后减速板振动试验

某型飞机后减速板在部队使用中多次出现减速板梁断裂、蒙皮裂纹等故障 ,打孔加型材结构改进方案经实际飞行测试取得了满意效果。为给出打孔加型材结构改进方案的使用寿命 ,进行了 2种结构后减速板的地面振动对比试验。本文对后减速板地面振动对比试验方法进行简要介绍。     

飞机起落架故障数据库模型与实现方法研究

讨论了民用飞机起落架故障数据库的结构模型，基于关系模型故障数据库故障树存储结构的表示及实现，详述了Treeview的基本功能和使用方法等内容。文章最后介绍了采用VFP建立Boeing737起落架故障数据库的部分功能。     

综合控制系统研究及其仿真

研究了综合火力/飞行/推进控制系统原理及其各个子系统的控制律设计方法,研究通过飞行、推进、火控等系统的综合实现自动飞行、自动攻击的原理,并利用VC 和Open GL联合开发了综合控制仿真、设计平台,结合有效的任务管理及控制律剪裁,实现了灵活的系统运行配置,将设计平台和仿真平台集为一体,并将多个系统的综合、测试、仿真在一个平台上实现。最后通过数字仿真表明,综合控制系统明显地提高了飞机综合化、自动化水平,也验证仿真平台达到了设计要求。     

航空发动机叶片三维强化抛光技术

针对我国航空涡轮发动机钛合金叶片强化抛光的现状,通过理论建模动力学分析计算,设计并试制出无导轨支承的三维振动强化抛光设备。三维振动强化抛光是一种新的强化抛光加工技术,通过试验证明,该技术解决了航空涡轮发动机钛合金叶片强化抛光的加工难点。     

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.     

一种新型旋转超声复合磨削头的研制

在分析传统超声波加工和超声波加工机床局限性的基础上,研制了一种新型的旋转超声复合磨削头,它可以安装在普通机床上,适用于硬脆材料及复合材料的加工。