基于回转体CAD/CAPP结构的图形文件OpenGL处理技术研究

在计算机辅助车削加工自动编程系统中,利用CAD软件系统输入图形,并通过应用程序对其文件格式进行转化,变成CAPP模块所需的基于特征的数据结构。     

液氮纯度分析的偏差及修正

液氮纯度是液氮产品非常关键的一个技术指标.液氮纯度的在线跟踪测量是通过测量液氮中的氧含量来实现的.在多年来的液氮在线分析及液氮出库分析过程中,发现氧含量测量结果普遍偏低.本文通过理论分析及大量的实验数据,找到了数据产生偏差的原因,并给出了科学的修正办法,为以后液氮生产过程中更加有效地控制产品质量打下了基础.     

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.     

论在X射线探伤中曝光时间与管电压的关系

本文针对X射线探伤中曝光时间与管电压的关系以及曝光时间在探伤中的实际意义做了详尽分析，并提出了对于不同厚度的零件如何选择曝光时间的原则。     

喷射沉积制备Al-Zn-Mg-Cu合金大型坯组织性能的研究

利用Ospray公司的喷射沉积设备制备了Al11.3Zn2.4Mg1.1Cu合金,合金挤压成棒材后,经过固溶和时效处理,用万能材料实验机对其进行了力学性能测试,合金的抗拉强度为849 MPa、屈服强度为796 MPa,延伸率为3.3%.透射电镜和扫描电镜对拉伸试样微观组织的研究结果表明,合金微观组织中包括微米级晶粒和纳米级晶粒,合金的强化方式为纳米晶强化、固溶强化以及沉淀强化,拉伸试样的断口分析表明,合金的断裂方式主要为沿晶断裂.     

高超声速三维碳—碳烧浊流场的数值研究

本文针对高超声速再体的烧蚀现象 ,利用简单隐式TVD差分格式和激波捕捉法 ,数值求解三维化学非平衡Navier Stokes方程 ,其中化学模型是碳 碳 (C C)空气化学模型 ,考虑 12个化学组分和 31个化学反应过程 ,研究了C C烧蚀对再入体头部区域的壁面温度和热流分布的影响。为了计算效率和稳定性提出壁面条件显式处理的方法。对再入高度为 6 5km和速度为 8km/s的再入体头部区域烧蚀流场进行了数值模拟 ,用飞行迎角α =0°的计算结果与国外文献进行了比较 ,符合得较好。同时给出了三维小迎角α =5°的计算结果     

基于VXI总线的检测软件设计

基于VXI总线和虚拟仪器技术，研制开发了用于外场的模拟式电子控制器检测软件，并对软件开发的过程和要求进行了分析，重点解决了程序设计中的需求分析和模块化设计问题。     

具有自学习功能的机载火控系统故障诊断系统研究

研究了一种应用于机载火控系统的具有自学习功能的故障诊断系统.首先介绍了系统的总体结构;然后通过分析火控系统的结构建立了层次诊断模型,并通过示例对诊断系统中知识的表达方法、推理方法等问题做了详细的分析;最后详细描述了系统的自学习机制.应用具有自学习功能的故障诊断专家系统,可实现综合化机载火控系统的智能故障诊断.     

GH4169合金疲劳裂纹扩展性能的试验研究

本研究中对GH4169高温合金的疲劳裂纹扩展性能进行了试验研究。主要进行了400℃～600℃范围内的疲劳裂纹扩展试验．其中对GH4169环形锻件进行了室温下的疲劳裂纹扩展试验。结果表明，在400℃-600℃范围内，温度对GH4169高温合金疲劳裂纹扩展性能的影响很小，随温度上升，裂纹扩展速率稍有加快；优质成分对GH4169高温合金的疲劳裂纹扩展性能几乎没有影响，在相同温度下，YZGH4169与GH4169的疲劳裂纹扩展速率几乎一样；材料品种对YSGH4169高温合金的疲劳裂纹扩展性能有一定影响，YSGH4169锻件比棒材的疲劳裂纹扩展性能要好一些。     

起落架落震试验测试系统的现状及其发展

能动地我国起落架落震试验测试系统发展的现状进行分析，指出了落震试验测试系统所存在的问题，说明了未来的发展重点及方向。