升降平台跌落对起落架过载的影响

建立了升降平台跌落时起落架动力学模型,给出了描述缓冲支柱和轮胎力性能的数学公式,使之适用于起落架严重受载的情况;通过数值仿真研究了升降平台跌落时的直升机起落架过载。分析了升降平台跌落时起落架产生大过载的力学机理。升降平台从不同高度自由跌落时,机轮系留引起的起落架正过载相对增加量不超过10%,而系留情况下起落架回弹行程中的负过载比压缩行程中的正过载高得多。     

IEEE488总线在动量轮测试中的应用

叙述了资源卫星动量轮的一般结构和开环测试原理。详细介绍了应用ＩＥＥＥ４８８总线构成的动量轮开环性能自动测试系统。说明了这个自动测试系统的系统构成以及测试项目、测试流程和获得的测试结果。并据此提出这个系统在卫星研制工作中具有推广价值。     

轮盘应变疲劳寿命可靠性分析方法

为较准确评估应变疲劳寿命可靠性，通过引入两个相关随机变量对Coffin-Manson公式随机化，发展了一种轮盘应变疲劳寿命可靠性分析概率模型。对线性回归残差重新定义，使得到的回归参数不随坐标系的选取发生变化。采用响应面法和蒙特卡洛模拟相结合的方法获得轮盘危险点应变幅的分布，最后通过多次解非线性方程数值模拟得到轮盘危险点应变疲劳寿命分布及其可靠寿命。     

混合式壁面移动机器人横向移动机构及运动分析

 针对结构较复杂的椭球形壁面，提出了由两类不同移动机构组成的混合式壁面移动机器人，一类为框架移动式，实现沿壁面经线（纵向）的攀爬运动；另一类为浮动的轮轨驱动式，实现沿壁面纬线（横向）的运动，二者相互独立。重点介绍了轮轨式横向移动机构，分析了它的工作原理，根据工作环境的几何特征并结合DH法，对复杂约束环境下，机器人的横向运动进行了运动学分析，并进行了样机实验，结果表明通过控制两个驱动轮的角速度可以控制机器人横向运动的速度和姿态。     

减速器等效试车大纲瞬态循环次数的当量计算研究

直升机传动系统主、尾减速器等传动部件的寿命考核,大量采用等效试车方法进行,对试车大纲中的瞬态载荷循环次数的当量处理是编制大等效比试车大纲的主要困难。本文采用MINER线性累积损伤法则,提出了一种有效的处理方法。并在Z9国产化尾减速器的1:1长试大纲的编制和考核中得到成功的应用。     

一种分析轮式起落架直升机“舰面共振”的方法

 针对轮式起落架直升机，提供了一种“舰面共振”动力稳定性分析方法。首先，针对直升机在舰面上随舰船一起摇晃时左右起落架受载不对称的状况，近似采用受对称载荷产生对称变形、受非对称载荷产生非对称变形的方法计算了直升机的平衡状态；其次，根据轮式起落架轮胎和缓冲支柱刚度和阻尼共同作用的特点，结合轮式起落架的几何关系，采用复刚度的方法得出起落架作用于机体的刚度与阻尼；最后，用桨叶振动模态法对轮式起落架的直升机进行了不同旋翼升力卸载以及鱼叉系留与否的“舰面共振”动力稳定性计算分析，并通过算例得到验证。     

基于MSP430汽车防抱死制动控制器的设计

介绍了一种汽车防抱死制动系统控制器的设计。控制器以MSP430F149单片机为核心,根据防抱死制动系统的工作原理,利用轮速传感器,对轮速进行滤波、放大、整形等实现车轮速度的采集。采用基于车轮滑移率的防抱控制理论,根据车速、轮速来计算车轮滑移率。在硬件设计方面,根据系统选择了MSP430F149单片机,设计出信号输入回路、输出驱动回路、电源部分,给出了系统结构原理图。     

月球探测器姿态大角度机动的反作用轮控制

研究了月球探测器转速与控制力矩受限的姿态大角度机动问题。根据时间变尺度思想，提出了双回路反馈的姿态大角度机动控制方法。以某型月球控测器为例，对该方法进行了仿真验证。结果表明，利用该控制方法，可使探测器以期望的角速度转动，从而完成探测器的姿态大角度机动。     

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.     

进口流量对无管式减涡器流阻特性影响研究

为分析进口流量对压气机引气系统无管式减涡器压力损失的影响及无管式减涡器减阻效果,采用数值模拟与试验研究相结合的方法对无管式减涡器开展研究,并与直喷嘴模型进行了对比。模型试验验证了数值模拟方法的可靠性,通过数值模拟,建立了无管式减涡器流阻特性"S"形曲线三分区模型,分析了无管式减涡器各截面间压力损失及其占比随无量纲质量流量变化规律。在计算流量范围内,与直喷嘴模型相比,无管式减涡器平均可降低压气机引气系统压力损失约45.9%。在第二拐点处,共转盘腔内压力损失降低了96.44%,此时无管式减涡器减阻效果最佳,较直喷嘴模型压力损失降低了73.44%。