Kevlar/Nomex蜂窝夹层结构表面粘贴镀铜箔聚酰亚胺薄膜的工艺研究

文章对Kevlar面板Nomex蜂窝夹层结构表面粘贴镀铜箔聚酰亚胺薄膜的工艺进行了研究,分析了工艺特点、工艺流程、工艺难点,以及针对工艺难点所采取的工艺措施,最后根据产品的研制情况给出结论。     

从应变计现状看电阻式传感器的前景

电阻式传感器的核心部件——电阻应变计是目前最常用的应力分析的敏感元件。也常用于测量力、压力、扭矩和加速度等物理量。作者简要回顾了电阻应变计的发展历史，介绍了电阻应变计的结构、分类及现状，展望了电阻式传感器的前景。     

柔性环境中的多目标决策及应用

提出了解决柔性环境中的多目标决策的一种人机交互式方法，该方法包括两个层次：（１）运用ｍａｘｉｍｉｎ方法进行优化；（２）根据决策者的愿望调整参数，再回到（１）。在计算机上实现了以上方法，并将该方法应用于修水县的扶贫规划。     

复合冷却结构冷却效率的试验研究

本文从主次流气动参数(相对静压降、主次流温比、主流马赫数等)和冷却结构(冲击高度、开孔率等)两方面比较分析了两种双层壁复合冷却结构及对应的单层壁冷却结构的冷却效率。试验结果表明:气动参数中相对压降对冷却效率的影响较大,结构参数中冲击高度对冷却效率的影响较小,而试验孔板开孔率对冷却效率的影响较大,增加冲击板后的双层壁复合冷却结构冷却效率大大增强。     

AB型聚酰亚胺单体的合成及气相沉积聚合研究

合成了三种AB型聚酰亚胺单体:4-(4-氨基苯氧基)邻苯二甲酸(单体4),4-(3-氨基苯氧基)邻苯二甲酸(单体7)和对(间)乙基4-(3-氨基苯氧基)邻苯二甲酸酯(单体8或9)。利用热失重分析(TGA)对比研究了这三种AB型聚酰亚胺单体的热行为。结果表明,单体4、单体7和单体8(9)在升温的过程中能发生热聚合生成聚酰亚胺。将单体4用于气相沉积聚合设备,得到了均匀透明的聚酰亚胺薄膜。对分子结构的修饰使单体8(9)较之单体7有更好的挥发性。     

冷轧机补偿原理及其控制算法

液压压下控制系统是冷连轧机控制系统中十分重要的组成部分,它主要实现机架辊缝大小的控制,对于轧制板材的板形有着直接的影响.在轧制过程中,由于轧辊偏心(包括工作辊和支撑辊)、油膜厚度的波动、轧机的弹跳等因素.为了解决这些问题,对于液压压下控制系统中存在的偏心补偿、油膜补偿和弹跳补偿进行了深入的理论分析,研究了冷连轧机液压压下控制系统中偏心补偿、油膜补偿、弹跳补偿的数学模型、实现过程,并与国内外相关理论进行了对比,阐述了各自的优缺点.     

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.     

逆向射流多斜孔气膜冷却的数值模拟

为了使航空燃气轮机燃烧室在高于燃烧室材料许用温度的前提下能够正常工作,需对燃烧室内壁采取冷却措施,并对变吹风比和变角度下的逆向射流多斜孔气膜冷却进行了数值模拟。在贴体坐标下划分网格,采用k-ε模型模拟湍流流动,求解气膜冷却过程的数学模型。分别改变逆向射流同主流的夹角,使其为20°、30°、45°和60,°改变吹风比的变化范围为0.5到1.5等多种条件下,对多斜孔气膜冷却效果进行了数值模拟。在所研究的范围内得到了符合规律的结论。研究结果表明,当吹风比不变的情况下,减小逆向射流角度,用有效温比表示的冷却效果相应提高。当逆向射流角度不变时,增加吹风比,冷却效果也相应提高。     

大型挠性充液卫星的动力学模型

研究了带有多个挠性附件和液体燃料贮箱的中继卫星系统的动力学建模问题。给出了微重力下小幅线性晃动等效模型基本参数，用混合坐标法描述中继卫星系统的构形，利用虚功原理推导出的矩阵形式的中继卫星动力学模型简洁且具有一般性，适用于许多开链飞行器系统。     

高能CO2激光腔镜高反介质薄膜的传输特性

为了获得适用于高能CO2激光器的高抗破坏阈值高反薄膜,以10.6μm高反膜ZnSe/YbF3,PbTe/BaF2膜系为例,数值模拟了激光在高反介质膜中的传输的场特性;给出了激光在多层介质膜中的场强分布、温度场分布及热应力分布。结果表明硅镜基体上的PbTe/BaF2膜系所需膜层厚度小、膜层数少,反射率可高达99.98%。