模拟服役环境中航空导管连接件耐蚀性能研究

采用自制的航空导管连接件腐蚀试验系统,研究了航空镀镉45^#钢导管连接件在模拟服役环境中的气密性、油压气密性以及应力腐蚀、表面腐蚀等性能.对该导管连接件在高温盐水溶液6%NaCl(90±5)℃浸泡与空气烘烤(60±5)℃循环200次条件下的表面腐蚀及应力腐蚀行为进行了评价;探讨了在模拟服役环境中,45^#钢发生腐蚀的机理.10^＃航空油不对镀镉45^＃钢造成腐蚀.镀镉45^#钢导管连接件在模拟服役环境中只是表面镀镉层发生腐蚀破坏,基体45^#钢只发生轻微腐蚀,表明45^＃钢导管连接件表面的镀镉磷化层可作为阳极性镀层而对基体金属进行保护.在最小屈服强度0.85的弯曲应力水平作用下,无应力腐蚀倾向.导管材料铝合金LF2-M与连接件45^#钢在6％NaCl水溶液中只有很小的电偶腐蚀电流,平均电偶电流密度为0.185μA/cm²,证明该类导管及导管连接件能安全地进行偶接.     

高强阻尼铝合金的阻尼性能和组织稳定性

采用时效处理实验,研究了快速凝固/粉末冶金工艺制备的X7093/5(Zn-30Al)高强度阻尼铝合金的阻尼性能和组织稳定性.将阻尼铝合金分别在50℃,100℃,120℃保温10?h,50?h,100?h后空冷,采用动态力学热分析仪(DMTA)和透射电镜(TEM)分别测试其阻尼性能和观察微观组织的变化情况.研究结果表明: 阻尼铝合金在时效过程中,组织结构由最初细碎杂乱的晶态结构转变为具有规则晶界的大晶粒结构,晶界对合金阻尼性能的贡献增强.在室温至250℃的温度范围内,合金阻尼值由4×10^-3增至3.0×10^-2.阻尼铝合金在120℃以下、100?h以内的时效处理中,时效温度和时效时间的不同对合金阻尼性能的影响不显著,材料的阻尼性能稳定性良好.     

模拟地热水温度对镀锌钢管腐蚀与结垢的影响

针对地热水环境中金属管道常见的腐蚀与结垢问题,采用扫描电子显微镜、能谱仪、X射线衍射仪等研究了不同温度的模拟地热水中镀锌钢管的腐蚀与结垢行为.结果表明:实验前期镀锌钢管的表面出现两种形貌("球"状和"针"状),不同温度的地热水中腐蚀与结垢产物的晶体形状不同,产物成分主要为Zn(OH)2,ZnO,CaCO3和MgCO3;镀锌钢管表面产物的分布对镀锌钢管在模拟地热水中的进一步腐蚀有一定程度的抑制;50℃地热水中的镀锌钢管表面的腐蚀坑面积较小,而在65℃和80℃地热水中腐蚀坑面积较大,镀锌钢管的腐蚀与结垢速度随地热水温度的升高而增大.     

含SiO2,ZrO2微粒复合镀镍层抗高温氧化性能

通过对含有SiO₂,ZrO₂微粒复合电沉积的研究,在Cu合金表面分别获得了含量(原子数分数)为11.3％ SiO₂,5.31％ ZrO₂微粒的Ni基复合镀层.通过在800℃、900℃条件下的高温氧化和热震循环试验,研究了这种复合镀镍层的高温氧化性能和界面结合特性.结果表明:经过40?h的高温氧化,2种复合镀镍层的抗氧化性能均达到抗氧化级,而且含SiO₂微粒的复合镀镍层的抗氧化性能优于含ZrO₂微粒的复合镀镍层;经过55次冷热循环,含SiO₂微粒的复合镀镍层与铜基体结合良好.     

溅镀C轴倾斜的压电膜和切变波谐振器

作者对溅镀的压电膜能否应用于甚高频至微波频率的声波器件进行了研究。本文介绍了切变波谐振器用的C轴倾斜的氧化锌(ZnO)和氮化铝(AlN)膜的生长及特性。文中计算了某些膜的切变波激动的定向关系。这些膜在C轴取向与表面法线成大约45°时,可能激励出接近于纯的切变波。在其他角度,则只能激励准切变波和准纵向波。 C轴对膜法线倾斜方向合适的ZnO或AlN膜,是在配有辅助阳极的反应式直流面磁控管溅镀系统中生长的。这类膜可用扫描式电子显微镜(SEM)和体声波器件测量法进行鉴定。自Si基片法线倾斜的C轴晶粒柱形结构可在扫描式电子显微镜中清楚地看到。C轴倾斜角达45°,厚度达10微米的薄膜已经制做成功。在P~+Si基片上溅镀上ZnO和AlN可以制成复合谐振器。这类谐振器的Q值在200兆赫到500兆赫基频谐振范围内大约为5000。特别令人感兴趣的是可以对谐振频率进行温度补偿。在ZnO/Si和AlN/Si的复合结构上已制造出室温下串联谐振频率的绝对温度系数小于1×10~6/℃的谐振器。ZnO和AlN晶片谐振器的温度系数已测出为-36.2×10~-6/℃和-25×10~-6/℃。这表明P~+Si基片在切变膜时的温度系数大约是+9×10~6/℃、     

氮化硼纳米片作为抗原子氧腐蚀填料的应用

对氮化硼纳米片(BNNS)作为填料提高聚合物的抗原子氧腐蚀性能进行了实验研究.利用液相剥离在聚乙烯醇(PVA)水溶液中制备了稳定分散的BNNS,采用基于离心技术的尺寸筛选方法,获得了具有3种不同横向尺寸的BNNS,其平均面积分别约为21.4,4.1, 1.0 μm2.采用浇注法,将PVA/BNNS分散液原位复合成复合薄膜.原子氧腐蚀实验表明:3种 BNNS均能提高PVA的抗原子氧腐蚀性能,添加约1.0 wt%的BNNS(平均面积为21.4 μm2) 可使质量损失降低87%.BNNS对原子氧的成键和壁垒效应,是其提高抗原子氧腐蚀性能的主要原因.      

再生型壳与ZTC4熔体的界面稳定性

从研究再生型壳中几种典型金属离子对铸件表面的污染影响规律入手,通过在型壳材料中添加Al、Nb和Mn等金属元素实际浇铸ZTC4合金（Ti-6Al-4V）,探讨不同残留金属在铸造过程中对铸件表面质量、陶瓷/钛合金界面成分、组织形貌及显微硬度等的影响,揭示废弃型壳材料中铸造残留金属对钛合金新铸坯陶瓷/合金界面稳定性的影响规律。结果表明:含Al、Nb和Mn等金属残留的型壳浇铸ZTC4合金,铸件表面外观平整无明显铸造缺陷;相比无金属残留型壳,含残留金属型壳的铸件表面粗糙度明显增加;Al金属残留对型壳与熔融钛合金界面稳定性的影响较小,而Nb和Mn金属残留能明显降低型壳与熔融钛合金的界面稳定性,铸件表面粗糙度可以在一定程度上反映界面稳定性;当型壳中含有Al金属残留时,陶瓷/合金界面处析出Ti₅Si₃相。      

航空用油介质和NaCl溶液中钛合金电化学特性

采用动电位扫描法研究了Ti-6Al-1.5Cr-2Zr钛合金在3#煤油和928滑油等高阻值油介质中的电化学极化特性.对于该新型钛合金电极在这2种航空油介质中自腐电位、极化电阻、腐蚀电流等电化学参数和相应的极化规律进行了研究.采用浸泡试验研究了该钛合金在3#煤油和928滑油中的腐蚀行为.结果表明钛合金在油介质中无明显腐蚀.对钛合金电极在高阻值油介质中电化学特性进行比较,研究了其在3.5%NaCl水溶液中的电化学行为,该钛合金电极在水溶液中的自腐蚀电位为-0.18V,在极化曲线上钝化区为0.27~1.24V,致钝电位为0.23V,致钝电流密度为0.31×10-4A/cm2.      

二维编织C/SiC复合材料板疲劳损伤分析

为探索复合材料损伤的基本规律,首先,基于损伤力学,结合Tsai-Hill强度理论,提出了表征二维编织C/SiC复合材料损伤各向异性的损伤演化方程;然后,在商业有限元软件ANSYS环境中进行了二次开发,形成了考虑材料刚度随损伤折减的损伤模拟程序;其次,对二维编织C/SiC复合材料板模型进行了损伤模拟分析,结果表明材料损伤过程中应力与损伤度对单元破坏起共同作用;最后,对损伤演化方程的形式提出了讨论与改进,并通过模拟计算揭示了复合材料在损伤驱动力及材料特性作用下损伤呈现各向异性演化的特征,说明材料各向异性损伤是其材料特性及受载形式产生的必然结果。      

Learning in an immersive digital theater

The Houston Museum of Natural Science, in collaboration with Rice University has an outreach program taking portable digital theaters to schools and community sites for over five years and has conducted research on student learning in this immersive environment. By using an external independent evaluator, the effectiveness of NASA-funded Education and Public Outreach (EPO) projects can be assessed. This paper documents interactive techniques and learning strategies in full-dome digital theaters. The presentation is divided into Evaluation Strategies and Results and Interactivity Strategies and Results. All learners from grades 3–12 showed statistically significant short-term increase in knowledge of basic Earth science concepts after a single 22-min show. Improvements were more significant on items that were taught using more than one modality of instruction: hearing, seeing, discussion, and immersion. Thus immersive theater can be an effective as well as engaging teaching method for Earth and Space science concepts, particularly those that are intrinsically three-dimensional and thus most effectively taught in an immersive environment. The portable system allows taking the educational experience to rural and tribal sites where the underserved students could not afford the time or expense to travel to museums.     

Stochastic particle acceleration by the forced interaction of relativistic current sheets

We address the problem of interacting relativistic current sheets in self-consistent kinetic plasma simulations within the framework of the Particle-In-Cell model. The interaction is enforced in head-on collisions of up to 10 current sheets at relativistic bulk speeds. The simulations are motivated by the general problem of Poynting flux dissipation in ‘striped wind’ configurations presumably governing the relativistic outflows pervasive in pulsar winds and gamma-ray bursts. We identify the generation of non-thermal particles and formation of a stable power-law shape in the particle energy distributions f(γ) dγ ∝ γ^−s dγ. In 1D, a spectral index s ∼ 2 is observed and attributed to a stochastic Fermi-type acceleration mechanism. In 2D, the generic index of s ∼ 3–4 is retained as in previous simulations of individual current sheets. Whereas in 2D the high energy cut-off is constrained by the limited dissipation of magnetic energy, in 1D the process converts the bulk motion of current sheets towards directed particle momentum of an exclusive class of non-thermal particles.     

基于LuGre模型的电液加载系统摩擦补偿

为了提高电液加载系统控制精度,针对摩擦问题提出了基于LuGre摩擦模型的前馈补偿方法.建立了用于摩擦仿真分析和补偿器设计的电液加载系统数学模型;通过实验获取并分析了相关的摩擦数据;基于实验数据进行LuGre模型参数辨识,把LuGre模型和辨识结果引入电液加载系统数学模型,并进行仿真结果与实际摩擦数据的对照,证明了LuGre摩擦模型的准确性.设计前馈补偿器,进行了实验对比,实验结果表明前馈补偿器可将摩擦产生的控制误差有效地降至未补偿时的30%左右.      

Concept options for the aerial survey of Titan

Various aerial platforms intended for long endurance survey of the Titan surface are presented. A few novel concepts are introduced, including a heated methane balloon and a balloon with a tethered wind turbine. All the concept options are predicted to have lower scientific payload fractions than the Huygens probe. It is concluded that the selection of the best aerial platform option depends on more accurate mass estimates and a clear decision on whether, or not, in situ surface composition measurements are required in conjunction with aerial remote sensing.     

Heterogeneous solid/gas chemistry of organic compounds related to comets,meteorites, Titan,and Mars: Laboratory and in lower Earth orbit experiments

To understand the evolution of organic molecules involved in extraterrestrial environments and with exobiological implications, many experimental programs in the laboratory are devoted to photochemical studies in the gaseous phase as well as in the solid state. The validity of such studies and their applications to extraterrestrial environments can be questioned as long as experiments conducted in space conditions, with the full solar spectrum, especially in the short wavelength domain, have not been implemented. The experiments that are described here will be carried out on a FOTON capsule, using the BIOPAN facility, and on the International Space Station, using the EXPOSE facility. Vented and sealed exposition cells will be used, which will allow us to study the chemical evolution in the gaseous phase as well as heterogeneous processes, such as the degradation of solid compounds and the release of gaseous fragments.     

CoRoT and Kepler results: Solar-like oscillators

The space-borne observatories CoRoT (Convection Rotation and planetary Transits) and Kepler have provided photometric time series data of unprecedented precision for large numbers of stars. These data have revolutionized the fields of transiting exoplanets and asteroseismology. In this review some important asteroseismic results obtained using data from the CoRoT and Kepler space missions concerning stars that show solar-like oscillations are discussed. These results comprise, among others, measurements of the location of the base of the convection zone and helium second-ionization zone in main-sequence stars, the presence (or not) of core-helium burning in red-giant stars, as well as differential rotation in these stars.     

HELIO: The Heliophysics Integrated Observatory

Heliophysics is a new research field that explores the Sun–Solar System Connection; it requires the joint exploitation of solar, heliospheric, magnetospheric and ionospheric observations.     

Radioactivity of the Moon and planets

In this report the main results of the study of radioactivity of the solar sistem bodies are considered. The radioactivity of the Moon and planets was measured by means of vehicles in situ. The radioactivity of the lunar samples, brought to the Earth was studied with laboratory equipment.     

The ESA scientific programme

The ESA scientific programme has, so far, provided several significant astrophysics experiments and further important missions are scheduled for execution during the next decade. These missions are briefly summarised together with several astrophysics investigations presently under study.     

应用于毫米波反射计的多项式校准方法

为了在毫米波波段准确测量波导器件的反射系数,提出了一种应用在反射系数测试前端(反射计)中的校准方法.该校准方法采用基于多项式的误差模型,使得每一个误差项的求解都转化成一个求解轨迹圆圆心的问题,同时不影响求解精度.采用一个滑动负载、一个滑动短路和一个短路器,在毫米波波段降低了对标准件理想程度的要求.实验中搭建了一个Ka波段的反射计,图解误差项的求解过程,分析了误差项的物理意义.把校准后的测量结果与商用矢量网络分析仪(VNA,Vector Network Analyzer)进行比较,吻合较好.同样比较了一组W波段反射计对波纹喇叭的测量结果,进一步验证了方法的合理性.