腐蚀对sic/Al(L2)和sic/Al-Ni复合丝力学性能的影响~①

本文对SiC/Al(L2)和SiC/A1-Ni复合丝在蒸馏水和在3.5％NaCl溶液中的耐腐蚀性能进行了研究。通过测试腐蚀前后复合丝的抗拉强度,利用气相色谱、发射光谱、X射线衍射等手段分析腐蚀气体和腐蚀产物,观察金相和扫描电镜下形貌的变化,发现SiC/A1复合丝在室温蒸馏水中36天、50℃和75℃蒸馏水中各15天浸泡后,其抗拉强度基本保持不变,说明该类复合材料对潮湿环境具有良好的耐腐蚀性能;SiC/A1-Ni复合丝在3.5％NaC1溶液中浸泡后,其抗拉强度随溶液温度升高和时闻延长而逐渐下降;其腐蚀主要是选择性腐蚀,其次是孔蚀和缝隙蚀。     

Instability and unsteadiness of aircraft wake vortices

This paper presents a review of theoretical and experimental results on stability and other unsteady properties of aircraft wakes. The basic mechanisms responsible for the propagation and the amplification of perturbation along vortices, namely the Kelvin waves and the cooperative instabilities, are first detailed. These two generic unsteady mechanisms are described by considering asymptotic linear stability analysis of model flows such as vortex filaments or Lamb–Oseen vortices. Extension of the linear analysis to more representative flows, using a biglobal stability approach, is also described. Experimental results obtained using LDV, hot wire and PIV in wind tunnels are presented and they are commented upon the light of theory.     

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.     

卷筒钢丝绳松弛实验研究

对提升机卷筒钢丝绳的应力松弛现象进行了实验研究 ,由此建立了卷筒钢丝绳的粘弹性本构关系 ,其结果对于提升机卷筒的结构设计有着重要的指导意义     

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。     

燃气二次喷射推力矢量控制系统启动过程非定常效应研究

采用数值模拟方法对燃气二次喷射推力矢量控制系统启动过程中非定常效应进行了研究.给出了详细的喷流瞬态干扰流场结构, 以及喷流瞬态干扰区随时间改变的流场细节特性,分析了流动参数和发动机内弹道性能的动态变化过程.研究表明,主/次流干扰流场内流动参数的分布及变化呈现复杂的多样性,启动过程中所呈现出的动态特性与系统稳定工作时有着明显的差异,侧向控制力、燃烧室平衡压强和发动机推力均有显著变化.在飞行器设计中,必须从安全控制的角度出发,考虑这一非定常效应的影响.     

固体冲压发动机喷管用C/C-SiC复合材料

采用"化学气相渗透+先驱体浸渍裂解"(CVI+PIP)混合工艺制备固体冲压发动机用C/C-SiC复合材料喷管内层,综合考查复合材料的微观结构、弯曲性能和抗烧蚀性能以及固冲发动机C/C-SiC喷管内层水压和点火实验。结果表明:复合材料的弯曲强度达到197 MPa,且断裂破坏行为呈现典型的韧性模式;复合材料具有优异的抗氧化烧蚀性能,氧化烧蚀200 s后线烧蚀率仅为0.0063 mm·s-1;研制的C/C-SiC复合材料构件的水压爆破压强为6.5 MPa,表明构件具有良好的整体承载能力;C/C-SiC复合材料喷管内层高温综合性能通过了固体冲压发动机点火实验考核。     

AZ31B镁合金双道次热变形过程流变应力特征模拟研究

建立了一类镁合金双道次热变形过程的二维元胞自动机模型。考虑到镁合金具有六重对称的密排六方晶体结构,模型采用了六边形元胞网格。另外,通过计算位错密度演变和设定晶粒形核长大规则,模型将热变形过程中动态再结晶、静态回复、静态再结晶、亚动态再结晶和晶粒长大等单个物理过程耦合到一起。为了验证模型,将其应用到AZ31B镁合金单道次和双道次热压缩过程。探讨了不同变形温度、应变速率、道次间隔和预应变对应力-应变曲线的影响。将计算结果和实验结果进行了对比,吻合较好。     

基于热态叶型的小轮毂比弯掠叶片结构保形设计与优化

发展了一种保持且基于气动设计给定的热态叶型的冷态叶型迭代解算方法,并将其融入叶片罩量调节的优化设计,其中在热态叶型的基础上调节罩量,针对冷态叶型计算变形与应力等,变形后的叶片逼近热态叶型,尽可能减小了对热态叶型气动特性的影响.实现了冷态叶型迭代求解与罩量调节中结构有限元网格的自动更新,并基于iSIGHT优化平台,建立了叶片罩量调节多目标优化设计的自动化分析流程,并以一小轮毂比弯掠风扇叶片罩量调节为例,考查了罩量调节中考虑轮盘与否对优化设计结果的影响.计算分析实例表明:所发展的方法可在保持热态叶型的前提下使叶片最大应力和最大变形分别下降了10.6%和46%.      

钛合金电弧增材制造技术研究现状及发展趋势

电弧增材制造技术作为增材制造的一个重要分支,在最近几年取得了显著的进展。文中简要介绍了增材制造技术的分类及各自特点,综述了钛合金电弧增材制造技术的研究现状,重点从钛合金成形零件的宏观和微观组织结构、制件显微组织控制方法两方面分析研究新进展,探讨了钛合金电弧增材制造技术发展所面临的技术问题以及需要重点考虑的发展方向。