计算机在固体火箭发动机设计与研制中的应用

随着计算机在分析与仿真中的广泛应用,固体火箭发动机工作过程中许多复杂而难以观察的现象已能得到揭示.因此,计算机的应用已成为设计与研制高性能固体火箭发动机的十分重要的手段.本文综述了应用计算机在一些固体火箭发动机的性能预示、设计优化、性能检验和故障分析等方面所取得的成就,并就今后我国在设计与研制固体火箭发动机中如何加强计算机化提出了若干建议.     

起落架落震试验的数字模拟方法

 <正> 在计算飞机起飞、着陆和滑行等地面运动的静、动态载荷时,除了需要飞机结构和气动参数外,起落架减震器的性能参数更占有重要地位。而这些性能参数中尤以决定油液阻尼力的流最系数为重要。长期以来,国内主要靠查手册、凭经验确定这个系数,如果能较准确地确定流量系数,对载荷计算是很有意义的事。     

两级固体火箭联合动力装置的参数优化

本文针对某型导弹由两级固体火箭发动机组成的联合动力装置进行九变量寻优计算.通过采用二维抛物线插值方法及合理组织迭代的技巧,解决了庞大的目标函数计算子程序耗时太多的问题;经大量调试,协调寻优步长、罚因子、收敛精度,最后成功地完成了本文的九维寻优计算,得到了能稳定收敛的最优解.所得最优方案比原参考方案的发动机总重减轻7.03kg(约占总重的2%).     

飞行控制系统虚拟原型技术

 在综述虚拟原型技术的基础上,研究飞行控制系统虚拟原型机以及采用虚拟原型技术后飞控系统的设计方法。提出了飞控系统设计,特别是飞控计算机设计中,基于虚拟原型技术的 3个层次应用,分析了构筑虚拟原型机需要重点解决的一些问题。     

电磁继电器、接触器可靠性试验系统的硬件设计

本文论述了电磁继电器、接触器可靠性试验系统的结构、功能及特点。描述了试验系统的硬件设计及相应的元器件选取原则；阐述了系统实现控制的方法。     

VB6.0在分布式监控系统数据通信中的应用

介绍一种采用VB语言编程,实现分布式监控系统数据通信的方法,讨论了通信协议及 编程要点,并给出程序。     

基于解析及特征造型的涡轮冷却叶片参数化设计

基于数学解析与特征造型技术相结合的方法,建立了基于构造过程的复杂涡轮冷却叶片的参数化设计技术。用五次多项式描述叶身型线,根据壁面厚度函数求解冷却通道外形,定义冷却通道隔板位置及厚度等参数,计算得到叶身及冷却通道各截面造型数据;以特征造型方法完成对涡轮冷却叶片转弯流道、缘板、榫头及叶片相关特征的参数化设计;利用CAD系统的二次开发接口,实现了多腔回流式涡轮冷却叶片的自动建模。     

基于Solid Works和Cosmos的模具结构三维设计及有限元分析

复杂结构注塑模具的设计和强度、刚度分析是注塑行业的重要难题。利用Solid Works三维设计软件实现了注塑模具的三维实体建模，并运用COSMOS／Works软件对注塑模具的典型部件进行了有限元分析，验证设计的零件是否符合实际工作情况是实现注塑模具现代化设计的重要途径。通过GearTrax2001Plus、Toolbox等外挂、内挂插件的使用．大大地简化了建模过程，克服了原有设计方法的不足．为解决较复杂的结构设计和理论分析问题提供了一种新的途径。     

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.     

航空涡喷、涡扇发动机强度设计系统

介绍了由发动机强度设计规范及准则、强度设计软件及方法、强度设计数据库及准则库构成的航空涡喷、涡扇发动机强度设计系统。用该系统可进行发动机构件的应力、振动和寿命分析。