液体压力激波加工技术研究

机械产品的零部件，通常需要通过成形与改性才具有所需形状及实用功能，本文提出了一种新型材料成形与改性加工的方法——液体压力激波加工。采用脉冲超声波聚焦技术，通过压电陶瓷激波发生器在液体介质中产生高能瞬时压力激波，对材料进行冲击，产生变形或表面改性。经过理论研究和试验验证，初步掌握了液体压力激波的产生、激波能量的控制和激波加工的动力学机制。这种加工方法具有能量可控性好、成本低廉和安全高效等优点，非常适合具有复杂结构和型面的中小零件加工，是一种颇具竞争力的先进制造技术手段。     

金属膜片贮箱膜片变形的数值模拟与失效分析

根据弹塑性有限变形理论，用有限元法建立了卫星推进系统贮箱金属膜片变形的有限元分析模型。在一定条件下，模拟了贮箱金属膜片的变形翻转过程，分析其翻转的特点，以及变形过程中表面压力、顶点径向位移和卷边处应力的变化，并给出了膜片失效原因。研究表明，数值模拟与试验结果较为吻合，所建分析模型合理。     

板料成形的数值分析及程序系统

本文讨论了板料成形的数值分析方法,并介绍一个能在微机上运行的程序系统——CASF(Computer Aided Sheetmetal Forming)01系统。 CASF01系统采用参数三次样条描述板金零件的几何外形,按弹-塑性流动理论用完全拉格朗日有限元法计算成形过程中的应力应变分布。由于参数样条的插值性和分段描述特点与有限元法的结构离散在基本思想和处理方法上的相似性,系统内曲面描述和力学分析程序间数据传递迅速方便。圆板胀形及其汽车零件的计算实例表明了CASF01系统的可靠性和实用性。     

摄影景深控制的几个技术问题

本文论述了三种景深控制形式与艺术内容表现、艺术价值创造的关系。     

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.     

Plastic wrinkling prediction in thin-walled part forming process:A review

The precision forming of thin-walled components has been urgently needed in aviation and aerospace field. However, the wrinkling induced by the compressive instability is one of the major defects in thin-walled part forming. The initiation and growth of the wrinkles are interac-tively affected by many factors such as stress states, mechanical properties of the material, geometry of the workpiece and boundary conditions. Especially when the forming process involves compli-cated boundary conditions such as multi-dies constrains, the perturbation of clearances between workpiece and dies and the contact conditions changing in time and space, etc., the predication of the wrinkling is further complicated. In this paper, the current prediction methods were summa-rized including the static equilibrium method, the energy method, the initial imperfection method, the eigenvalue buckling analysis method, the static-implicit finite element method and the dynamic-explicit finite element method. Then, a systematical comparison and summary of these methods in terms of their advantages and limitations are presented. By using a combination of explicit FE method, initial imperfection and energy conservation, a hybrid method is recommended to predict plastic wrinkling in thin-walled part forming. Finally, considering the urgent requirements of com-plex thin-walled structures’ part in aviation and aerospace field, the trends and challenges in wrin-kling prediction under complicated boundary conditions are presented.     

钣金成形信息化发展关键技术

钣金成形广泛应用在航空、汽车、船舶等各个行业,而钣金成形信息化在钣金成形技术中起重要作用.钣金成形信息的存储方式、关联技术、信息规范技术、数据库技术、钣金成形信息共享平台技术、钣金成形信息的获取和利用技术,是钣金成形信息化的关键技术.通过这些关键技术规范钣金成形信息的表达、存储方式,建立完善的钣金成形信息平台,利用数据挖掘技术,为钣金成形技术人员提供钣金成形工艺方案、工艺规程、模具设计需要的充足的信息.钣金成形信息化技术的发展将理顺钣金成形信息的积累和利用,消除信息孤岛,提高钣金成形的整体工艺水平和工艺准备效率.     

新型Al-Li-Cu-Mg合金蒙皮拉伸成形特性试验研究

随着新型Al-Li-Cu-Mg合金蒙皮在航空航天等高技术工业的应用日益广泛,新型Al-Li-Cu-Mg合金蒙皮拉伸成形特性已成为新型Al-Li-Cu-Mg合金板蒙皮成形质量精确控制以及蒙皮设计迫切需要解决的关键问题.因此,首先获得了新型T8态Al-Li-Cu-Mg合金的最佳热处理工艺参数;其次,采用试验方法,研究了不同热处理状态的拉伸成形过程,揭示了新型Al-Li-Cu-Mg合金板材的拉伸成形特性.发现通过固溶处理,后续时效能够显著提高新型T8态Al-Li-Cu-Mg合金材的拉形能力;在新型A1-Li-Cu-Mg合金板材拉形过程,桔皮现象主要出现在补拉阶段,蒙皮悬空区应变值＞0.0215时,板材表面将出现桔皮,且与材料热处理状态无关.     

热压罐和RTM成型的C型框弯曲试验研究

通过热压罐和RTM成型工艺的复合材料C型框弯曲试验,研究了两种工艺方法对其承载能力及破坏模式的影响.试验结果表明:热压罐成型的隔框承载能力比RTM成型工艺高27.5％,且其分散性小;两种工艺的破坏位置一致,但RTM成型的隔框在平直段与弯曲段过渡截面处外壁先发生分层,而热压罐成型在该处外壁至破坏前才出现分层损伤.该结论可以为该型结构的工程应用提供有价值的参考.     

可重复使用热防护材料应用与研究进展

可重复使用热防护系统是为高速重复使用飞行器而发展的关键性技术,涵盖了地球大气环境及非地球大气环境下的弹道式再入、高马赫数巡航等应用场景。根据现有高马赫数飞行器热防护现状,对高马赫数飞行器的主要热防护系统类型、特点和使用场景进行了简要介绍。在此基础上,结合国外里程碑式可重复使用飞行器（X-15、SR-71、航天飞机、X-33、X-37B、Spaceliner等）,梳理了可重复使用热防护材料的应用与研究进展,论述了代表性可重复使用热防护材料的发展、性能、研制进度、特点及应用前景。对国外在可重复使用热防护材料研制中的设计及发展思路,以及所存在的主要问题进行了总结归纳,为可重复使用热防护材料未来的发展提供了思路。