接触角法测玄武岩及玻璃纤维表面能实验

通过Wilhelmy吊片法测试液体与玄武岩、玻璃纤维单丝的前进接触角,应用OWRK理论计算得到纤维表面能及其色散与极性分量.实验研究表明:未经表面处理的玄武岩纤维表面能高于S-2玻璃纤维,去除浸润剂后2种纤维表面能的极性分量均明显降低,并且测试液体的极性分量对纤维表面能的测试结果影响甚大.分析结果为纤维与树脂的表面张力合理匹配、形成良好界面浸润和粘接提供了理论依据.      

基于虚拟现实技术的无人直升机实时监控系统

引入虚拟现实技术,结合遥测数据的快速有效滤波和插补方法形成可视性和可靠性良好的无人直升机远程实时监控系统.有效地提高飞行状态显示形象性,动态性,遥测数据的可靠性和实时性.使离机驾驶员对无人直升机的控制更加直观有效,提高飞行任务成功率.      

SMARC变形控制及神经网络建模

在复合材料层板中偏离中性层的位置铺设镍钛形状记忆合金丝,然后通电加热镍钛丝,使其在形状回复过程中产生巨大的回复力,从而使层板结构发生弯曲变形.由于形状记忆合金的非线性以及合成的智能材料结构的应力、应变分布和形状变化规律都非常复杂,尝试引入人工神经网络来建立以可控参量(电流强度)为输入变量、易测参量(稳态挠度)为输出变量的模型,所建模型的预测数据与实验数据之间符合得较好,相对误差小于9%.      

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.     

Orbital phase spectroscopy of four high mass X-ray binary pulsars to study the stellar wind of the companion

Our work focuses on a comprehensive orbital phase-dependent spectroscopy of the four High Mass X-ray Binary Pulsars (HMXBPs) 4U 1538-52, GX 301-2, OAO 1657-415 and Vela X-1. We hereby report the measurements of the variation of the absorption column density and iron-line flux along with other spectral parameters over the binary orbit for the above-mentioned HMXBPs in elliptical orbits, as observed with the Rossi X-ray Timing Explorer (RXTE) and the BeppoSAX satellites. A spherically symmetric wind profile was used as a model to compare the observed column density variations. Out of the four pulsars, only in 4U 1538-52, we find the model having a reasonable corroboration with the observations, whereas in the remaining three the stellar wind seems to be clumpy and a smooth symmetric stellar wind model appears to be quite inadequate in explaining the data. Moreover, in GX 301-2, neither the presence of a disk nor a gas stream from the companion was validated. Furthermore, the spectral results obtained in the case of OAO 1657-415 and Vela X-1 were more or less similar to that of GX 301-2.     

含多处任意脱层层合梁屈曲的微分求积解法

基于铁木辛柯(Timoshenko)梁理论,建立了含任意脱层的复合梁模型,并利用微分求积DQ(Differential Quadrature)法,研究了含多处任意脱层层合梁的屈曲问题.该复合梁模型给出的含单脱层层合梁的临界屈曲载荷计算结果与相关文献结果一致.此外,以两端固支,含两个任意长度、任意深度贯穿脱层的层合梁为例,分析了脱层长度、深度以及相对位置对屈曲载荷的影响.为工程结构设计和分析提供了一种简单有效的方法,给出了一些有参考价值的结果.     

循环湿热环境下碳纤维复合材料的界面性能

针对CCF300/5428复合材料在循环湿热环境下的吸湿-脱湿行为和层间剪切性能进行了研究,并结合扫描电镜观察了循环湿热处理的不同阶段纤维/基体界面结合状态.研究结果表明:经过反复吸湿后,水分的初始扩散速率和饱和吸湿率增加;脱湿后水对复合材料层间剪切性能的影响大部分可以消除;复合材料吸湿后室温环境下性能下降较少,但在高温高湿环境下,复合材料的性能会显著降低.     

基于G2的卫星控制系统故障诊断的半物理仿真

研究一种基于G2的集故障注入、故障模拟和故障诊断为一体的半物理仿真系统,包括基于VxW orks的实时硬件模拟系统、星载姿轨控计算机、数管及遥控遥测模拟器和专用接口箱等.开发了基于G2的以某一类典型卫星控制系统为对象的故障诊断专家系统,并对G2外部接口进行了扩展设计.最后,以典型故障为例,在半物理仿真平台上进行了演示验证.     

“嫦娥二号”卫星L2点角动量管理

对“嫦娥二号”(CE-2)卫星进入环绕日地拉格朗日L2点的李萨如轨道后卫星喷气卸载所产生的影响进行了研究.提出了一种利用光压力矩辅助卫星太阳电池翼角度调整进行角动量管理的方法.在轨试验表明,太阳光压强度足够对飞行在L2点环绕轨道上的CE-2卫星进行角动量管理,可以大幅度减少动量轮在轨喷气卸载的次数,有利于CE-2卫星的轨道维持.     

Comparison of ionosphere characteristic parameters obtained by ionosonde with IRI-2007 model over Southeast Asia

In this work, the foF2 and hmF2 parameters at the conjugate points near the magnetic equator of Southeast Asia are studied and compared with the International Reference Ionosphere (IRI) model. Three ionosondes are installed nearly along the magnetic meridian of 100°E; one at the magnetic equator, namely Chumphon (10.72°N, 99.37°E, dip angle 3.0°N), and the other two at the magnetic conjugate points, namely Chiang Mai (18.76°N, 98.93°E, dip angle 12.7°N) and Kototabang (0.2°S, 100.30°E, dip angle 10.1°S). The monthly hourly medians of the foF2 and hmF2 parameters are calculated and compared with the predictions obtained from the IRI-2007 model from January 2004 to February 2007. Our results show that: the variations of foF2 and hmF2 predicted by the IRI-2007 model generally show the similar feature to the observed data. Both parameters generally show better agreement with the IRI predictions during daytime than during nighttime. For foF2, most of the results show that the IRI model overestimates the observed foF2 at the magnetic equator (Chumphon), underestimates at the northern crest (Chiang Mai) and is close to the measured ones at the southern crest of the EIA (Kototabang). For hmF2, the predicted hmF2 values are close to the hmF2(M3000F2_OBS) during daytime. During nighttime, the IRI model gives the underestimation at the magnetic equator and the overestimation at both EIA crests. The results are important for the future improvements of the IRI model for foF2 and hmF2 over Southeast Asia region.