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。     

高强度铝合金中氢传输的研究

采用化学镀镍层作为铝合金LC4上防护层,应用电化学氢渗透技术研究了氢在LC4中的静态传输规律以及在不同热处理状态下,氢在LC4中的传输对其应力腐蚀敏感性的影响。实验结果表明:常温下氢在LC4中的静态传输是以扩散为控制步骤的过程。氢扩散系数为10~(-9)cm~2·s~(-1)数量级,为同条件下氢在纯铝中扩散系数的四分之一;LC4材料的DCB试样在常温下的3.5％NaCl溶液中的应力腐蚀断裂不遵循氢脆机理。     

LC9高强度铝合金过时效工艺试验

通过对ＬＣ９高强度铝合金过时效工艺试验，并与ＬＣ９ＣＳ状态作性能对比，证实该材料具有良好的耐应力腐蚀及抗裂纹扩展性能，从而确认ＬＣ９ＣＧＳ３铝合金在飞机上推广使用的可行性。     

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.     

BH新型憎水剂及其憎水膜层“三防腐蚀”性能研究

研究了BH系列(BH 102和BH 103)憎水剂的合成工艺、技术指标、憎水处理成膜工艺以及憎水膜层的憎水效果和耐腐蚀性能。结果表明,BH系列憎水剂的憎水效果良好,在零件表面形成的憎水膜层能达到105°以上的憎水角;同时经BH系列憎水剂处理后的钢铁磷化表面的耐腐蚀性能得到明显改善,具有优良的"三防腐蚀"性能,其中含有复配缓蚀剂的BH 103憎水膜层的耐腐蚀性更优于添加单一缓蚀剂的BH 102憎水膜层。     

常温腐蚀对Al-Si涂层氧化行为的影响

研究了未经 /经常温腐蚀的 DZ1 2 5镍基合金表面 Al-Si涂层的高温氧化行为。结果表明 ,经腐蚀的涂层等温氧化行为发生变化。在初始阶段 ,经腐蚀的试样增重大于未经腐蚀的试样 ,而且经腐蚀的试样的耐高温性能明显下降。氧化皮中主要是 Al2 O3及少量的 Ti O2 .     

电沉积CeO2/Zn纳米复合涂层

将纳米氧化铈颗粒加入镀锌液中进行复电沉积制得纳米复合涂层。通过失重法，ICP，SEM和XRD方法探讨了纳米氧化铈颗粒对电沉积锌涂层的影响。结果表明，在同样的电沉积条件下，纳米复合涂层的耐蚀性明显提高，而微米复合涂层的耐蚀性只稍有改善；纳米复合涂层中氧化铈的含量高于微米复合涂层中的氧化铈含量。纳米氧化铈颗粒改变了锌涂层的表面组织形貌和晶体结构，从而提高了涂层的耐蚀性。     

基于幂函数模型的民机结构腐蚀扩展寿命评定方法研究

基于飞机结构腐蚀清除后测量获取的腐蚀深度,提出了飞机结构腐蚀扩展寿命的幂函数动态预测模型以及模型参数定义方法,确定了腐蚀条件下的飞机结构腐蚀扩展寿命评定指标,建立了基于运营状态下飞机结构腐蚀信息更新的民用飞机结构腐蚀扩展寿命评定方法。     

基于损伤检测的飞机结构腐蚀损伤预测方法对比研究

针对飞机结构材料易腐蚀特点,采用 BP 神经网络算法、数据拟合方法、指数平滑预测三种方法,对飞机铝合金结构腐蚀损伤进行预测对比分析。预测结果及其误差以及对比分析图表明,BP 神经网络算法所构建的网络预测模型对一定腐蚀周期内的腐蚀损伤有较好预测能力,指数平滑预测方法和幂函数数据拟合方法对一定腐蚀周期之外的腐蚀损伤预测有较好的外延性。     

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。