民用飞机机翼副油箱静载荷计算

以亚音速、大展弦比的大中型民用飞机机翼挂装副油箱为研究对象,分析CCAR-25部中载荷计算的相关适航条款内容,考虑外挂物自身运动及机翼结构弹性变形对副油箱气动载荷的影响,给出了副油箱静载荷计算的过载—速度包线,高度—速度包线、载荷计算情况等,在工程应用成熟的《运输类飞机载荷计算程序包》基础上,采用亚音速稳态定常流升力线理论与风洞试验相结合的方法,将机翼简化为悬臂梁进行气动弹性修正,开展副油箱气动力弹性修正计算、惯性力计算、副油箱质量实时更新、包线筛选等功能模块的研究,通过工程应用其计算精度满足要求,形成了满足适航条款的副油箱静载荷计算方法,规范了副油箱静载荷的计算流程,拓展了《运输类飞机载荷计算程序包》的功能。     

纳米压痕法测试压痕蠕变的应用研究

阐述压痕蠕变的研究进展及其测试原理,并且采用纳米压痕仪对Ta,Ni和Ni基高温合金三种金属体材料、BaTiO3陶瓷和Ag/Co多层薄膜进行蠕变实验,分析蠕变应力指数和相应的蠕变机制.     

Ti3Al基合金室温拉伸形变机制的研究

在透射电子显微镜上，利用双倾双束技术和不可见判据，分析了Ｔｉ－２５Ａｌ－１０Ｎｂ－３Ｖ－１Ｍｏ（ａｔ－％）合金中具有ＤＯ１９结构的α２相在室温拉伸形变时的位错类型和滑移系。证明，α２相在室温拉伸形变时，主要开动的是型位错的滑移系，例如＜１１２０＞｛１１００｝＜１１２０＞｛０００１｝和少量以位错对存在的型位错滑移系，如＜１１２６＞｛２０２１｝。     

气泡和液滴在上升或下降时大变形的数值模拟

本文在考虑界面张力的条件下用涡片方法导出了二维无粘气泡和液滴在另一种静止无粘流体中上升或下降时运动和变形的支配方程，提出了求解支配方程的数值方法，并在数值模拟的例子中研究了空气泡和煤油滴在水中上升时及水滴在煤油中下降时的变形规律，研究了数值模拟中界面张力对界面形状的影响，气泡上升的数值模拟结果与相应的试验结果基本一致。数值模拟结果表明本方法可正确模拟饣泡和液滴在上升或下降过程中的大变形，直到界面发     

关于厚薄板弯曲分析的内位移杂交元法

 本文通过引入单元内位移和优化处理的单元应力场,以计入剪切变形的板弯曲能量泛函为基础,导出适用于厚、薄板分析的四边形杂交应力元。内力场和内位移的合理选择避免了单元零能模式的出现、避免了解的剪切自锁现象。该优化单元显示了较好的通用性和收敛性。对关于剪切自锁的RCI判据提出了反例、说明了它的局限性。     

等温锻造Ti—47Al—2Cr—1Nb合金显微组织细化机理

Ti 4 7Al 2Cr 1Nb(at % )合金经等温锻造形变热处理后 ,显微组织得到显著细化 ;TEM分析表明 ,TiAl合金在等温变形时 ,形变主要以γ相板条内产生变形孪晶的方式进行 ;大部分变形孪晶垂直于α2 /γ界面 ,热处理时易形成再结晶核心 ,形成等轴γ晶粒     

基于残余应力分布的框类零件装夹方案优选的有限元模拟

 非均匀分布的残余应力是引起工件变形的主要原因。为了揭示装夹方案对残余应力的影响,利用有限元技术模拟了工件加工过程中不同的装夹方案,并分析了模拟结果。结果表明,装夹位置对残余应力分布具有重要影响,而装夹顺序对残余应力的分布和幅值无较大影响。通过进一步对比分析各种装夹方案中残余应力引起的工件变形得出结论:夹具分布较平均的装夹方案可获得比较均布的残余应力和较小的变形。     

内螺旋花键冷挤压成形工艺

介绍了某产品齿轮挡块 45°内螺旋花键的冷挤压成形工艺，包括模具设计及试验过程。     

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.     

飞机整体结构件加工变形的有限元模拟与试验研究

在模拟淬火、拉伸过程获得含有初始残余应力的预拉伸板材以及模拟单齿切削过程获得切削载荷的基础上,提出并采用接力算法,对一航空整体结构件的材料铣削过程进行有限元仿真,同时进行了试验研究.结果表明,有限元模拟的整体结构件的变形与试验具有一致性,从而证明提出的整体结构件加工仿真关键技术的可行性,避免了为研究加工变形而进行的繁琐的试错法.