二元推力矢量喷管导流管的设计研究

针对某型飞机进行二元推力矢量改装时对发动机出口的气流进行过渡转换的问题，设计了喷管导流管，将导流管气流截面由圆形过渡到长方形。本文利用有限元软件PATRAN对导流管进行了应力强度分析和变形分析，得出导流管的应力分布场和变形位移场，通过对不同厚度的导流管的分析计算得出导流管最大应力和最大位移随管壁厚度变化曲线，从而确定最佳的管壁厚度。研究了导流管最大应力和最大位移沿轴向的变化曲线，并对导流管的结构进行了优化设计，给出两种优化设计方案，得到较为理想的结构。     

Indicators of black-hole mass and Eddington accretion ratio from QSO X-ray and UV spectra

The evolution of luminous QSOs is linked to the evolution of massive galaxies. We know this because the relic black-holes found locally have masses dependent on the properties of the host galaxy’s bulge. An important way to explore this evolution would be to measure dependences of black-hole masses and Eddington accretion ratios over a range of redshifts, i.e., with cosmological age. For low redshift QSOs (and their lower luminosity Seyfert galaxy counterparts) it has been possible to infer black-hole masses from the luminosities and velocity dispersions of their host-galaxy bulges. These masses agree with those virial black-hole masses calculated from the Doppler widths of the broad Hβ emission lines. The latter method can then be extended to more distant and luminous QSOs, up to redshifts of 0.6 with ground-based optical observations. We discuss ways to extend these explorations to higher redshifts – up to 3 using the widths of QSOs’ broad UV emission lines, and in principle, and to redshifts near 4 from ground-based infrared observations of rest-frame Hβ at 2.5 μm. We discuss the possibility of investigating the accretion history of the higher redshift QSOs using measures of Eddington accretion ratio – the soft X-ray spectral index and the eigenvectors of Principal Components Analyses of QSOs’ UV emission-line spectra.     

高旋转数下45°斜肋回转通道平均换热特性研究

为了更加深入地研究涡轮叶片回转通道的换热特性,研究了高旋转数下带45°斜肋回转通道的平均换热特性。在通道进口雷诺数从10000~70000,旋转数从0~2.07的范围内,实验研究了旋转状态下,方形截面带45°斜肋U型通道径向出流与径向入流两个流程四个侧面在0°,22.5°和45°三个安装角下的平均换热系数。研究结果表明:45°斜肋增强了通道换热,减弱了旋转对换热的影响;由于浮升力作用在肋间二次流上,导致通道内外侧出现临界回流现象;转角减弱了第一通道旋转对换热的影响,增强了第二通道旋转对换热的影响,其影响在低旋转数下并不显著,在高旋转数下开始变得明显。     

三应答器SINS/USBL紧耦合导航算法

SINS/USBL组合导航误差因素主要包括USBL测距精度误差、USBL测角误差、USBL到SINS的安装误差以及应答器的位置误差,且现有USBL设备的普遍特点为:测距精度高而测角精度相对较差。针对上述误差因素和特点,提出一种三应答器SINS/USBL紧耦合导航算法,避免了USBL测角误差以及USBL到SINS的安装角误差等对导航精度的影响,仿真结果表明能够较大程度上提高组合导航定位精度。此外,该算法无需对安装角进行标定,使用更加便捷。     

时域有限体积法的格式稳定性分析

以模型方程为例,采用MUSCL插值的S-W通量分裂格式,分别结合二步、四步龙格一库塔时间推进格式建立数值求解方法.用Von Neumann傅里叶级数分析方法,通过对不同格式的放大因子及色散因子的计算,分析了时域有限体积法(FVTD)格式的稳定性.     

直升机旋翼标准桨叶的选定原则与方法研究

本文对直升机桨叶单片互换的原理进行了论述，对标准桨叶的确定原则以及实施方法进行了探讨，并结合直11型机标准桨叶选定工作的流程和结果，对所述方法进行了实例分析。     

Multi-channel discharge characteristics cutting by ultra-fine wire-EDM

Compared with a copper wire electrode, molybdenum wire with a poor conductor is usually used as the electrode in high speed wire-cut electrical discharge machining(HSWEDM), so the resistance of an ultra-fine wire cannot be ignored. To study the differences of discharge characteristics between the ultra-fine wire and the conventional diameter wire, the continuous discharge waveform of two kinds of wire electrodes was compared. It was found that there was a multichannel discharge phenomenon in the...     

非牛顿流体粘度测试方法及标准物质研究进展

本文介绍了常用非牛顿流体粘度的测量方法如毛细管法、旋转粘度计法、旋转流变仪法等,对流变仪校准方法和非牛顿流体粘度标准物质的国内外研究进展情况进行了综述,并对未来非牛顿流体粘度标准物质的发展趋势进行了预测和展望。     

小卫星非常规动力学分析与控制

针对小卫星研制中出现的一些非常规动力学问题进行研究,并提出解决办法。针对小卫星组件最大冲击谱量级超出常规冲击试验规范谱的分析与验证困难,通过研究提出了能够分析评估组件高量级冲击的方法。针对小卫星随机振动下强度设计方法还存在较大误差,分析了系统模态质量比与模态频率在一定频段的影响规律,认为忽略模态质量耦合会带来误差,提出了考虑模态质量耦合的准静态载荷计算方法。最后,针对小卫星整星开展了减振研究,分析了正弦和随机减振效果,对于对称安装减振系统,提出了减振系统的主频率计算公式。     

一种模拟视频信号亮度对比度校准方法

本文针对模拟视频信号长距离传输后信号衰减和偏移的问题,提出一种软件自动校准的方法。通过分析源端发送的校准图样,调整视频AD芯片的增益和偏移参数,达到最佳的亮度和对比度校准效果。