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.     

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.     

The effects of CO2 on growth and transpiration of radish (Raphanus sativus) in hypobaria

Plants grown on long-term space missions will likely be grown in low pressure environments (i.e., hypobaria). However, in hypobaria the transpiration rates of plants can increase and may result in wilting if the water is not readily replaced. It is possible to reduce transpiration by increasing the partial pressure of CO₂ (pCO₂), but the effects of pCO₂ at high levels (>120 Pa) on the growth and transpiration of plants in hypobaria are not known. Therefore, the effects of pCO₂ on the growth and transpiration of radish (Raphanus sativus var. Cherry Bomb II) in hypobaria were studied. The fresh weight (FW), leaf area, dry weight (DW), CO₂ assimilation rates (C_A), dark respiration rates (DR), and transpiration rates from 26 day-old radish plants that were grown for an additional seven days at different total pressures (33, 66 or 101 kPa) and pCO₂ (40 Pa, 100 Pa and 180 Pa) were measured. In general, the dry weight of plants increased with CO₂ enrichment and with lower total pressure. In limiting pCO₂ (40 Pa) conditions, the transpiration for plants grown at 33 kPa was approximately twice that of controls (101 kPa total pressure with 40 Pa pCO₂). Increasing the pCO₂ from 40 Pa to 180 Pa reduced the transpiration rates for plants grown in hypobaria and in standard atmospheric pressures. However, for plants grown in hypobaria and high pCO₂ (180 Pa) leaf damage was evident. Radish growth can be enhanced and transpiration reduced in hypobaria by enriching the gas phase with CO₂ although at high levels leaf damage may occur.     

航天器可测试性设计研究

在调研国内外可测试性技术发展历程的基础上,分析中国航天器可测试性设计技术与国外的差距,探讨其发展的前提条件和规划方法,提出适合中国航天器的可测试性设计的技术实现途径.