弹载引信电控扫描识别目标方位的方法

研究了弹载引信电控扫描识别目标方位的一种方法，该方法是：首先研究一种周期电控脉冲起动单刀四掷微波开关，该开关又逐次起动可瞄准定向天线的每一元和它们的公共收发系统。因而该系统既能全向搜索空中目标，又能分区截取回波信号，由此获得引信天线电控扫瞄形式的可瞄准探测系统。     

用于激光推进的球隙火花开关放电特性的研究

在自行研制的高压球隙火花开关上,研究短间隙下(6 mm)不同工作气压、不同冷却气体速度对开关工作电压范围、延迟时间和抖动时间的影响及规律。结果表明:提高气压能扩大工作电压范围,增加开关的时延;吹气能够降低开关的时延,但增加开关的抖动时间。在本实验条件下,将开关工作气压从1×105Pa提高到2×105Pa,工作电压范围扩大了50%以上,但开关的时延增加了20 ns,抖动增加了10 ns;有气体冷却时开关的延迟时间比起无吹气时要小几十个纳秒。     

开关磁阻调速电动机的运行控制

 开关磁阻调速电动机（SRD）是由双凸极型磁阻电动机、功率逆变器、转子位置检测器、定子绕组电流检测器以及运行控制器等部件组成的系统。它可以看作是大步距角、带位置闭环控制的步进电机的一种发展。 SRD结构如图1（α）所示。为避免磁拉力,定、转子齿数均为偶数。在各定子齿上设有集中绕组,正对两齿上的绕组联成一相。考虑电机出力,结构合理及定子绕组供电频率等因素,一般采用定子齿数比转子齿数多2个的结构。图中是所研制的定子8齿、转子6齿的样机结构（简称为8/6结构）。图1（b）为功率逆变电路。其中C_s为直流电源,T₁～T₄为四相绕组主开关,D₁～D₄为相应的续流二极管。     

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.     

某起落架正常收／放系统失效原因分析

正确运用246雷达天线“正常或应急”液压操纵开关和液压马达壳体回油“正常或应急”开关的工作状态，关系到飞机液压操纵系统的安全性。若天线液压操纵开关和马达壳体回油开关配合不当，将引起飞机液压操纵系统失效。     

双框架飞机蒙皮检测机器人切换运动控制方法

针对一种双框架飞机蒙皮检测机器人,通过分析该机器人在飞机表面上的受力情况,在飞机表面该机器人受到了非完整约束,基于牛顿-欧拉法建立了机器人非完整约束动力学模型。根据机器人机械结构和运动步态分析,将该非完整机器人系统分为子系统A和子系统B。为了实现机器人在飞机表面运动,采用反演技术和快速Terminal滑模控制相结合的思想对系统设计了控制器,提出了一种反演-滑模控制方法;对于非完整机器人子系统A和子系统B,设计了一种基于事件驱动的切换策略,实现了机器人对期望轨迹的全局渐近跟踪,并利用Lyapunov稳定性证明系统的跟踪误差收敛。仿真和试验表明,采用该切换策略和反演-滑模控制方法,双框架飞机蒙皮检测机器人可以在飞机表面自由运动并进行损伤检测,具有良好的可靠性和稳定性。     

可重复使用热防护材料应用与研究进展

可重复使用热防护系统是为高速重复使用飞行器而发展的关键性技术,涵盖了地球大气环境及非地球大气环境下的弹道式再入、高马赫数巡航等应用场景。根据现有高马赫数飞行器热防护现状,对高马赫数飞行器的主要热防护系统类型、特点和使用场景进行了简要介绍。在此基础上,结合国外里程碑式可重复使用飞行器（X-15、SR-71、航天飞机、X-33、X-37B、Spaceliner等）,梳理了可重复使用热防护材料的应用与研究进展,论述了代表性可重复使用热防护材料的发展、性能、研制进度、特点及应用前景。对国外在可重复使用热防护材料研制中的设计及发展思路,以及所存在的主要问题进行了总结归纳,为可重复使用热防护材料未来的发展提供了思路。     

齿冠形收敛喷管模型气动和红外辐射特性数值研究

针对齿冠形收敛喷管的气动和红外辐射特性进行了数值计算,并与常规收敛喷管进行了对比.在本文研究范围内的结果表明:①齿冠形收敛喷管的推力损失大于常规收敛喷管;②齿冠形尾缘引射外界大气与主流掺混的能力强于常规收敛喷管,核心区长度得到有效衰减;③齿冠形喷管的热喷流3～5μm红外辐射强度在侧向相对常规收敛喷管的衰减量在15%左右,尾缘内倾角对于尾喷流红外辐射强度衰减的影响甚微;④齿冠内倾时,尾向处能遮挡喷管内部热部件.      

着陆襟翼打开状态下抓斗式反推装置 三维流动数值模拟

基于求解三维Reynolds-averaged Navier-Stokes方程,数值模拟了着陆襟翼打开状态下抓斗式反推装置工作时流场分布特性.网格采用非结构化四面体与六面体混合分区生成技术,湍流模型选用Spalart-Allmaras模型.结果表明,在计算滑跑速度范围内,反向排气流不会被进气道重新吸入;高温反向排气流会冲击到飞机吊挂及部分机翼,需引起注意;随着滑跑速度的降低,反向排气流侧向影响范围急剧增大,若机翼后掠角较大,则反向排气流容易被相邻发动机再次吸入,引起进气畸变;当滑跑速度降低到34m/s时,反向流开始吹向地面,可能会卷起地面颗粒物并且被进气道吸入;随着滑跑速度的降低,反推力减小.      

新型超高强Al-Zn-Mg-Cu铝合金热压缩变形的流变应力行为

采用热力模拟试验方法进行热压缩变形试验,研究了一种新型Al-Zn-Mg-Cu合金在变形温度为300～450℃,应变速率为0.001～1s-1,压缩变形程度为50%条件下的流变应力行为.结果表明,变形温度和应变速率对合金流变应力的大小影响显著,流变应力随变形温度的升高而降低,随应变速率的提高而增大.采用统计回归方法建立了...