LY2铝合金激光冲击处理实验研究

分析激光冲击处理技术及相对于传统强化方式的优点,针对LY2航空铝合金材料,设计进行试件激光冲击处理实验,通过对激光冲击处理前后材料性能的测试,分析激光冲击处理对LY2铝合金材料疲劳寿命、强度性能的影响.     

Magnetic and Optical Properties of the TiO2-Co-TiO2 Composite Films Grown by Magnetron Sputtering

The TiO2-Co-TiO2 sandwich films were successfully grown on glass and silicon substrata making alternate use of radio frequency reactive magnetron sputtering and direct current magnetron sputtering. The structures and properties of these films were identified with X-ray diffraction (XRD), Raman spectra and X-ray photoemission spectra (XPS). It is shown that the sandwich film consists of two anatase TiO2 films with an embedded Co nano-film. The fact that, when the Co nano-film thickens, varied red shifts appear in optical absorption spectra may well be explained by the quantum confinement and tunnel effects. As for magnetic properties, the saturation magnetization, remnant magnetic induction and coercivity vary with the thickness of the Co nano-films. Moreover, the Co nano-film has a critical thickness of about 8.6 nm, which makes the coercivity of the composite film reach the maximum of about 1413 Oe.     

Effects of RRA Treatments on Microstructures and Properties of a New High-strength Aluminum-Lithium Alloy-2A97

A new high strength 2A97 Al-Cu-Li-X alloy was subjected to triple-aging of retrogression and re-aging treatments (RRA). Transmission electron microscopy (TEM), differential scanning calorimetry (DSC), and tensile tests were used to investigate the effects of RRA treatment on the microstructures and properties. DSC test reveals the reversion temperature range of the strengthening δ' (Al3Li)phase. The results show that the microstructure consists of δ' (Al3Li) phase, T1 (Al2CuLi) phase and θ"/θ'(Al2Cu) phase for 2A97 alloy treated by a triple-aging ora retrogression and re-aging treatment in the following order: (1) at 165 ℃×30 min, (2) at 220 ℃ or 240 ℃×15 min, (3) at 165 ℃×24 h. The plastic deformation, incorporated into the treatment after secondary high temperature aging, promotes the T1 precipitation during final re-aging. The tensile properties of the alloy treated by the retrogression and re-aging treatment reach the peak level of alloy single-aged at 165 ℃ in T6 temper.     

KM6水平舱改造测控系统研制

宇航员出舱活动是我国载人航天发展战略的第二步——空间实验室工程的一项基本任务。为满足完成“SZ-7人-船-服”出舱活动联合试验任务的需要,必须需要对原有KM6水平舱进行适应性的功能改造。为了确保宇航员的生命安全,必须尽可能的提高整个控制系统的可靠性,。测控系统在总体结构上采用SIEMENS PCS7冗余集散控制系统的方式,对所有关键测控环节（包括控制计算机、CPU、电源、网络、I/O模块等）都进行了冗余备份,以确保宇航员出舱活动试验流程的顺利进行,并对重要操作中关键参数互联、互锁,杜绝误操作,确保有完善的系统监控和故障报警功能,。改造后通过多次调试和多种试验模式演练,各分系统和总控系统测控功能均达到设计指标要求。为人-舱-服联合试验提供了坚强的后盾。     

ECAP变形2J4合金回火后的磁性能研究

研究了磁性材料2J4合金经等径弯曲通道变形(Equal Channel Angular Pressing,简称ECAP)和不同温度回火后的磁性能,并与冷轧变形合金的磁性能进行了对比分析.结果表明,2J4合金随着ECAP变形道次的增加,磁导率增加,4道次ECAP变形的饱和磁感应强度最高.另外,2J4合金的磁性能对回火温度的变化非常敏感,呈波浪式变化.4道次ECAP变形2J4合金沿挤压面(S面)进行85%冷轧变形,在610℃回火后获得的磁性能最好,矫顽力达到3.8364 kA/m.ECAP变形2J4合金沿挤压面的磁性能远优于传统冷轧合金.试验结果证实了采用ECAP变形方式制备高性能磁性材料是可行的.     

浆料浸渍结合反应熔渗法制备2D C/SiC-Zr B_2复合材料

利用XRD,SEM,EDS研究浆料浸渍结合反应熔渗法制备2D C/SiC-ZrB2复合材料的组成与结构,并测定了复合材料的弯曲强度.结果表明:采用单向加压依次渗入ZrB2微粉和酚醛树脂,能很好地将ZrB2微粉和树脂渗入到纤维束间,但熔融Si难以渗入到试样内部,复合材料的开气孔率和室温弯曲强度分别为18.3%和110MPa.采用ZrB2浆料真空浸渍,沉积碳基体后进行熔融渗Si,复合材料的开气孔率和室温弯曲强度分别为5.5%和230MPa.     

无侧滑二元超声速进气道侧板遮挡度对其性能影响

针对某Ma_d=2.4矩形进口截面的二元混压式进气道,在Ma_∞=2.51及2.27条件下,数值研究了无侧滑角时侧板遮挡度对进气道性能的影响,获得了喉道处各性能参数随侧板遮挡度的变化关系并分析了其变化原因.研究表明:当侧板下端位于压缩面平直段后,各性能参数变化明显;对于所研究的进气道采用位置靠后的侧板有利于改善进气道的起动性能,但却大大增加了阻力也牺牲了流量系数.      

基于尺度共生矩阵的滚动轴承故障诊断研究

基于滚动轴承振动信号的各种三维或二维谱图中包含的不同故障信息的客观现实,通过二维小波变换在不同尺度空间下构造的小波共生矩阵提取了谱图的纹理特征向量.利用灰关联分析表征这些纹理特征的不同发展态势从而实现滚动轴承的故障诊断.对实测滚动轴承不同状态故障数据的分析表明:该方法具有较高的故障模式分类精度;随着故障尺寸的增加,由于轴承各部件的相互影响诊断正确率会有所降低.同时研究表明对于特定的诊断方法是否进行特征向量归一化需区别对待.      

Variation of ionospheric electron and ion temperatures during periods of minimum to maximum solar activity by the SROSS-C2 satellite over Indian low and equatorial latitudes

To study the variation of ionospheric electron and ion temperatures with solar activity the data of electron and ion temperatures were recorded with the help of Retarding Potential Analyzer payload aboard Indian SROSS-C2 satellite at an average altitude of ∼500 km. The main focuses of the paper is to see the diurnal, seasonal and latitudinal variations of electron and ion temperatures during periods of minimum to maximum solar activity. The ionospheric temperatures in the topside show strong variations with altitude, latitude, season and solar activity. In present study, the temperature variations with latitude, season and solar activity have been studied at an average altitude ∼500 km. The peak at sunrise has been observed during all seasons, in both electron and ion temperatures. Further, the ionospheric temperatures vary with latitude in day time. The latitudinal variation is more pronounced for low solar activity than for high solar activity.     

Ionospheric variation at Thailand equatorial latitude station: Comparison between observations and IRI-2001 model predictions

In this paper, the F2-layer critical frequency (foF2) and peak height (hmF2) measured by the FM/CW ionosonde at Thailand equatorial latitude station, namely Chumphon (10.72°N, 99.37°E, dip 3.22) are presented. The measurement data during low solar activity from January 2004 to December 2006 are analyzed based on the diurnal, seasonal variation. The results are then compared with IRI-2001 model predictions. Our study shows that: (1) In general, both the URSI and CCIR options of the IRI model give foF2 close to the measured ones, but the CCIR option produces a smaller range of deviation than the URSI option. The agreement during daytime is generally better than during nighttime. Overestimation mostly occurs in 2004 and 2006, while underestimation is during pre-sunrise hours in June solstice in 2005. The peak foF2 around sunset is higher during March equinox and September equinox than the other seasons, with longer duration of maximum levels in March equinox than September equinox. Large coefficients of variability foF2 occur during pre-sunrise hours. Meanwhile, the best agreement between the observed foF2 and the IRI model is obtained in June solstice. (2) In general, The IRI (CCIR) model predicts the observed hmF2 well during daytime in June solstice from 2004–2006, but it overestimates during March equinox, September equinox and December solstice. For nighttime, the model overestimates hmF2 values for all seasons especially during March equinox and September equinox. However, the model underestimates hmF2 values during September equinox and for some cases during June solstice and December solstice at pre-sunrise. The agreement between the IRI model and the hmF2(M3000_OBS) is worst around noontime, post-sunset and pre-sunrise hours. All comparative studies give feedback for new improvements of CCIR and URSI IRI models.