受轴向拉伸载荷作用的耳片强度研究

耳片是飞机结构的重要连接元件,是结构主要传力通道上的重要环节,是飞机结构强度计算和细节分析的重点部位。多年来,许多国内外学者、专家对其进行了大量试验研究工作。大量的试验表明,随着加载角度的增大,耳片的静拉伸破坏载荷降低,所以,现在在设计中,都尽量采用受轴向载荷的耳片。本文对受轴向拉伸载荷作用下的单、双耳片进行了强度分析研究,并进行了归纳总结。     

低膨胀高温合金的发展及在航空航天业的应用

回顾了低膨胀高温合金的发展历史."因瓦效应"和"时效硬化"现象的发现奠定了低膨胀高温合金发展的基础.20世纪70年代航空航天事业的迅猛发展以及能源危机的爆发为低膨胀高温合金在航空航天业的实际应用提供了宝贵的契机, 最早的商用Fe-Ni-Co(IN9××)系列合金,经过用Nb、Ti强化,去Al,加Si等一系列成分上的变化,显著改善其应力加速晶界氧化脆性(SAGBO性能),从此低膨胀高温合金在航空航天领域得到大量应用.为改善此类合金的抗氧化和降低裂纹扩展速率等性能,又进行了新合金系的研究,即以Inconel 783合金为代表的Fe-Ni-Co-Al-Cr系合金和以Haynes 242合金为代表的Ni-Mo-Cr系合金的研究,这些合金在750℃仍能达到完全抗氧化,为新一代飞机发动机的发展提供了优质材料.     

功率谱密度(PSD)在评价超精密光学表面中的应用研究

用原子力显微镜对不同工艺下获得的超光滑反射镜基片进行了功率谱密度(PSD)检测,并对结果进行分析,以指导光学元件加工。     

等离子体表面技术的研究与应用

概述了离子注入、离子束沉积、等离子喷涂、离子镀、等离子体增强化学气相沉积、等离子体化学热处理和双层辉光离子渗金属等等离子体表面技术的基本原理和最新进展,并给出了部分典型实例。     

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.     

基于散乱数据表面法矢的二次曲面拟合

 为了解决二次曲面拟合算法中因几何参数初值计算方法不精确而导致的求解效率低，甚至失败的问题，提出了基于表面法矢的二次曲面直接拟合算法。采用不同的模型对该方法与已有二次曲面拟合技术进行了性能对比测试与分析。在此基础上建立了二次曲面提取的方案,给出了散乱数据二次曲面提取的实例。实验与理论分析表明，文中方法可以精确求解二次曲面的几何参数的初值，从而提高了曲面拟合算法的性能，为逆向工程中的数据分割与特征提取提供了新的技术手段。     

卫星姿控发动机喷管羽流撞击效应试验

在高超声速低密度风洞中试验研究了卫星姿控发动机喷管羽流对平板模型的撞击效应,包括气动力和气动热效应。试验气体为加热的氮气。对两个卫星姿态控制发动机喷管的十种实验状态进行了测量。测出了平行于喷管轴线的平板模型上的压力分布和温度变化及处于喷管上方后流区的挡板的温度变化,给出了平板模型上的气动力和气动热分布规律,并判断是否形成后流区。测量结果表明,试验结果可靠,具有工程应用价值,能为姿控发动机在卫星上的布局提供参考。     

航空发动机风扇叶片两种表面处理方法对比

在对激光冲击强化技术与喷丸表面强化技术比较分析之后,表明航空发动机叶片经过激光冲击强化后,能显著增加叶片表面残余压应力,提高疲劳性能,并且其效果优于喷丸表面强化技术。     

三维舵面绕流的N-S方程计算研究

基于粘性非结构混合网格,采用格心格式的有限体积法,应用Spalart-Allmaras湍流模型进行绕三维舵面流动的N-S方程数值模拟。操纵面铰链力矩的计算结果与风洞试验结果的对比分析表明,计算方法对粘性流动具有良好的适应性。对舵面铰链力矩随迎角、马赫数、雷诺数变化的规律也进行了分析研究。     

纳米精度光学非球面研磨、抛光技术

介绍了高精度光学非球面的研磨、抛光技术与计算机控制水平、机械设计能力等相关领域的发展。