砂布轮柔性抛光力的建模与参数优化

砂布轮柔性较大可以实现航空发动机叶片微面切触自适应抛光,提高叶片表面完整性和力学性能。抛光力是影响抛光表面完整性的关键参数,通过单因素试验分析确定了砂布轮抛光力的影响参数及其影响规律,通过正交试验和极差法确定了影响抛光力的主要参数是砂布轮的压缩量和转速;利用二元二次回归正交试验得出了抛光力的预测模型,利用该模型分析了抛光力预测误差变化趋势,明确了不同转速下抛光力主要影响参数的稳定域;整体叶盘的抛光试验表明：通过合理控制抛光力,可以实现表面粗糙度小于0.4 μm的抛光效果,且效率比人工提高20%。     

煤油两相连续旋转爆震燃烧室工作特性试验研究

为了深入分析煤油燃料两相连续旋转爆震燃烧室的工作特性,采用富氧空气或氧气为氧化剂,通过试验得到爆震波的时域、频域特征,对两相连续旋转爆震燃烧室中爆震波的起爆过程和稳定后的传播过程进行研究。利用基于激光散射相位多普勒分析(PDA)技术对雾化流场进行了测量,得到喷注器出口不同平面处煤油液滴速度与直径的统计分布。试验结果表明当煤油流量为78g/s,氧气流量为224.0g/s,空气流量为72.5g/s,当量比为1.083时,燃烧室在单波模态下工作,爆震波传播频率为0.904k Hz,平均转速为649m/s。使用氧气作为氧化剂,当煤油流量为81.8g/s,氧气流量为231.8g/s,当量比为1.222时,燃烧室在双波模态下工作,爆震波传播频率为5.882k Hz,平均转速为1848m/s,传播过程中表现出很强的非定常性。在当量比为0.805~0.908的富氧工况下,随着氧化剂中含氧量的增加,爆震波的速度逐步增大,最终达到2440m/s;在当量比为1.057~1.220的富燃工况下,随含氧量的增加爆震波速度呈现线性增长的特征。     

Ionospheric response of equatorial and low latitude F-region during the intense geomagnetic storm on 24–25 August 2005

In this investigation, we present and discuss the response of the ionospheric F-region in the South American and East Asian sectors during an intense geomagnetic storm in August 2005. The geomagnetic storm studied reached a minimum Dst of −216 nT at 12:00 UT on 24 August. In this work ionospheric sounding data obtained of 24, 25, and 26 August 2005 at Palmas (PAL; 10.2° S, 48.2° W; dip latitude 6.6° S), São José dos Campos (SJC, 23.2° S, 45.9° W; dip latitude 17.6° S), Brazil, Ho Chi Minh City, (HCM; 10.5° N, 106.3° E; dip latitude 2.9° N), Vietnam, Okinawa (OKI; 26.3° N, 127.8° E; dip latitude 21.2° N), Japan, are presented. Also, the GPS observations obtained at different stations in the equatorial and low-latitude regions in the Brazilian sector are presented. On the night of 24–25 August 2005, the h′F variations show traveling ionospheric disturbances associated with Joule heating in the auroral zone from SJC to PAL. The foF2 variations show a positive storm phase on the night of 24–25 August at PAL and SJC during the recovery phase. Also, the GPS-VTEC observations at several stations in the Brazilian sector show a fairly similar positive storm phase on 24 August. During the fast decrease of Dst (between 10:00 and 11:00 UT) on 24 August, there is a prompt penetration of electric field of magnetospheric origin that result in abrupt increase (∼12:00 UT) in foF2 at PAL, SJC (Brazil) and OKI (Japan) and in VTEC at IMPZ, BOMJ, PARA and SMAR (Brazil). OKI showed strong oscillations of the F-region on the night 24 August resulted to the propagation of traveling atmospheric disturbances (TADs) by Joule heating in the auroral region. These effects result a strong positive observed at OKI station. During the daytime on 25 August, in the recovery phase, the foF2 observations showed positive ionospheric storm at HCM station. Some differences in the latitudinal response of the F-region is also observed in the South American and East Asian sectors.     

Future of Space Astronomy: A global Road Map for the next decades

The use of space techniques continues to play a key role in the advance of astrophysics by providing access to the entire electromagnetic spectrum from radio to high energy γ rays. The increasing size, complexity and cost of large space observatories places a growing emphasis on international collaboration. Furthermore, combining existing and future datasets from space and “ground based” observatories is an emerging mode of powerful and relatively inexpensive research to address problems that can only be tackled by the application of large multi-wavelength observations. While the present set of astronomical facilities is impressive and covers the entire electromagnetic spectrum, with complementary space and “ground based” telescopes, the situation in the next 10–20 years is of critical concern. The James Webb Space Telescope (JWST), to be launched not earlier than 2018, is the only approved future major space astronomy mission. Other major highly recommended space astronomy missions, such as the Wide-field Infrared Survey Telescope (WFIRST), the International X-ray Observatory (IXO), Large Interferometer Space Antenna (LISA) and the Space Infrared Telescope for Cosmology and Astrophysics (SPICA), have yet to be approved for development.     

航天器控制系统高可信度地面测试技术

随着航天器复杂程度和指标要求的不断提高,高可信系统级地面测试越来越凸显其重要性.以工程应用为出发点,对航天器控制系统高可信地面测试涉及的相关理论和技术进行探讨.提出了测试可信度的定义,并以航天控制工程为背景分析了测试可信度的影响因素.在此基础上,系统介绍了柔性化原型测试、航天器控制系统指标专项测试、高可信动力学建模、高可信信号源技术等方面的初步研究成果.     

Coronal fast wave trains of the decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare

The 22 min long decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare simultaneously by the Brazilian Solar Spectroscope (BSS) and the Ond?ejov radiospectrograph in frequency range 1200–4500 MHz has been analyzed. We have found that the characteristic periods of about 60 s belong to the long-period spectral component of the fast wave trains with a tadpole pattern in their wavelet power spectra. We have detected these trains in the whole frequency range 1200–4500 MHz. The behavior of individual wave trains at lower frequencies is different from that at higher frequencies. These individual wave trains have some common as well as different properties. In this paper, we focus on two examples of wave trains in a loop segment and the main statistical parameters in their wavelet power and global spectra are studied and discussed.     

三维全五向编织复合材料细观结构实验分析

对三维(3D)全五向编织复合材料的细观结构进行了实验研究,三维全五向编织复合材料是一种新型的编织复合材料,其细观结构对预测材料的性能有重要作用。采用显微计算机断层成像(micro-CT)技术得到了三维全五向编织复合材料的截面图片,通过在碳纤维试件中混编入少量玻璃纤维作为示踪纱,提高了示踪纤维束在截面图片中的的对比度。并通过三维重建得到纤维束实体模型,结合CAD技术对纤维束的横截面形状与空间走向进行了研究。结果表明:编织纱与轴纱纤维束的截面形状在材料不同区域与不同的花节高度内是变化的;在不同区域,编织纱的空间走向也是不同的;而轴纱在空间上基本保持伸直。由于编织纱对轴纱的挤压使轴纱表面产生螺旋状的压痕。      

基于AD736真有效值测量的发电机电压控制技术研究

针对电励磁同步发电机电压控制技术存在参数漂移、工作不稳定、电压畸变导致控制参数超差等诸多问题,介绍一种电励磁同步发电机数字电压控制技术,通过AD736高精度芯片测量交流电压真有效值,并采用基于双闭环数字PI算法的电压控制技术,开展了发电机电压数字控制器研制。经试验考核,该控制器性能指标满足设计要求,达到了预期目标。     

红外动态目标模拟器光学系统的设计

设计了一种用于红外导引头性能测试的红外动态目标模拟器,利用数字微镜阵列(DMD)对黑体红外辐射进行反射调制,并由光学准直系统实现红外场景生成系统与红外导引头的光学耦合。用光学设计软件（ZEMAX）对准直光学系统进行了设计和优化,准直光学系统成像质量良好,接近衍射极限,点列图直径小于艾里斑直径,畸变小于0.1%。结果表明该系统环境适应性强,能很好地用于红外导引头动态图像的校准。     

带摆镜的制冷型中波红外像方扫描光学系统设计

基本形式的像方扫描光学系统依然需要复杂的二维回转机构带动成像镜组做二维扫描,所以二维回转机构需要承担较大载荷。分析了基本形式的像方扫描光学系统形式,并在基本形式基础上加入摆镜,只通过二维摆镜的旋转达到扫描像面的目的,大大减小二维回转机构载荷,提高扫描速度,简化了系统结构,减小了系统体积。加入摆镜后的光学系统除具有基本形式像方扫描光学系统的性质外,还有了新的限制条件,对带摆镜的像方扫描光学系统进行了分析,提出了设计条件及设计方法,并设计出具有较大视场的像方扫描光学系统。