利用光学层析技术重构超声速绕流流场密度分布

在连续式风洞中,采用单光路旋转流场干涉测量和计算机层析方法获得了含模型的超声速绕流流场密度分布。首先利用多种图像处理方法,并引入计算机辅助功能,对干涉图片进行精确判读和定量处理,准确重构波前相位信息;获得了相应的PV值、RMS值以及前15阶的Zemike多项式系数;通过同原始CFD模型波前数据的对比,系统的重构精度RMS优于λ／10。在获得一系列单帧干涉波前相位数据的基础上,采用光学层析技术,设计计算机迭代算法,构造内部旋转矩阵,重构了超声速绕流流场密度分布,可以非常直观地获得待测流场不同方向截面上的密度分布状况。     

涡轮盘低循环疲劳寿命概率分析

大量试验证明疲劳寿命符合对数正态分布,并且对数寿命标准差随应变水平降低而增大;在此基础上,引入对数寿命的线性标准差及标准正态随机变量μ,将Mason-Coffin公式随机化,疲劳性能参数均表示为μ的函数,建立了基于试验数据统计分析的概率寿命模型.对GH4133材料疲劳试验数据进行线性异方差回归分析,得到了疲劳性能参数的随机表达式及概率密度曲线,各参数并不服从正态分布或对数正态分布.应用该模型对某涡轮盘进行了低循环疲劳寿命可靠性分析,获得了轮盘寿命分布,对应最大概率和可靠度0.9987的寿命均与轮盘的试验分析相吻合.     

利用光学层析技术重构超声速绕流流场密度分布

在连续式风洞中,采用单光路旋转流场干涉测量和计算机层析方法获得了含模型的超声速绕流流场密度分布.首先利用多种图像处理方法,并引入计算机辅助功能,对干涉图片进行精确判读和定量处理,准确重构波前相位信息;获得了相应的PV值、RMS值以及前15阶的Zernike多项式系数;通过同原始CFD模型波前数据的对比,系统的重构精度RMS优于λ/10.在获得一系列单帧干涉波前相位数据的基础上,采用光学层析技术,设计计算机迭代算法,构造内部旋转矩阵,重构了超声速绕流流场密度分布,可以非常直观地获得待测流场不同方向截面上的密度分布状况.     

边界层风洞主动模拟装置的研制及实验研究

研制可控振动尖劈在风洞中模拟湍流边界层,寻找一种简易可行的运动控制结构和方法,试验结果证明了尖劈的低频机械振动增强了相应频率的湍流能量,增大了湍流积分长度.     

电磁驱动液态金属热控系统分析

对电磁驱动液态金属热控系统进行了分析,与水工质回路的传热特性比较表明：在进行高功率密度器件散热方面,液态金属换热性能明显优于水等常规工质,在较小的流速下,可以保持较低的器件表面温度;更为重要的是,它可以采用无运动部件电磁泵驱动,具有可靠性高、振动噪声小、结构简单紧凑、功耗小、可控性强等优点。该系统不仅可解决空间高热流密度器件散热难题,而且在微小卫星、月球／行星表面探测器等主动热控制方面也有重要的应用前景。     

Multi-resolution Analysis of Density Fluctuation of Coherent Structures About Supersonic Flow over VG

The density field around a vortex generator (VG) in supersonic flow is studied with a nanoparticle-based planar laser scattering (NPLS) method. Based on the calibration, i.e., the density distribution of the supersonic flow around a wedge, the density field of a supersonic VG is measured. According to movement characteristics of coherent structure in VG’s flow fields and the basic concepts of wavelet, the density fluctuating signals and multi-resolution characteristics of density field images are studied. The multi-resolution characteristics of density fluctuation can be analyzed with wavelet transformation of NPLS images. The wavelet approximate coefficients of density fluctuating signals exhibit their characteristics at different scales, and the corresponding detail coefficients show the difference of diverse layer smooth approximation in some way. Based on 2D wavelet decomposition and reconstruction of density field images, the approximate and detail signals at different scales are studied, and the coherent structures at different scales are extracted and analyzed.     

限带高斯白噪声声压时程模拟的修正三角级数法

针对传统三角级数法模拟高声压级下的高斯白噪声声压有效值与理论值存在误差的问题,提出一种修正三角级数法,预先将各谐波振幅置为1,最后调整声压有效值为理论值,模拟过程简单,消除了传统方法模拟有效值与理论值之间的误差。数值模拟得到的声压时程数据准确可靠,具有良好的随机性,表明方法用于限带高斯白噪声声压时程模拟具有合理性、可行性。     

Modeling of sub-ionospheric VLF signal perturbations associated with total solar eclipse, 2009 in Indian subcontinent

During the total solar eclipse of 2009, a week-long campaign was conducted in the Indian sub-continent to study the low-latitude D-region ionosphere using the very low frequency (VLF) signal from the Indian Navy transmitter (call sign: VTX3) operating at 18.2 kHz. It was observed that in several places, the signal amplitude is enhanced while in other places the amplitude is reduced. We simulated the observational results using the well known Long Wavelength Propagation Capability (LWPC) code. As a first order approximation, the ionospheric parameters were assumed to vary according to the degree of solar obscuration on the way to the receivers. This automatically brought in non-uniformity of the ionospheric parameters along the propagation paths. We find that an assumption of 4 km increase of lower ionospheric height for places going through totality in the propagation path simulate the observations very well at Kathmandu and Raiganj. We find an increase of the height parameter by h^′=+3.0$h^{\prime }=+3.0$ km for the VTX-Malda path and h^′=+1.8$h^{\prime }=+1.8$ km for the VTX-Kolkata path. We also present, as an example, the altitude variation of electron number density throughout the eclipse time at Raiganj.     

Harmonic analysis of the ionospheric electron densities retrieved from FORMOSAT-3/COSMIC radio occultation measurements

In order to investigate the regular variations of the ionosphere, the least-squares harmonic estimation is applied to the time series of ionospheric electron densities derived from about five years of Global Positioning System radio occultation observations by FORMOSAT-3/COSMIC satellites. The analysis is done for different latitudes and altitudes in the region of Iran. The least-squares harmonic estimation is found to be a powerful tool for the frequency analysis of the completely unevenly spaced time series of radio occultation measurements. Although the obtained results are slightly different from the exact expected cycles (i.e. annual and diurnal components with their Fourier decompositions, and the 27-day period) due to the low horizontal resolution of radio occultation measurements, high vertical resolution of the observations enables us to detect not only the total electron content variations but also periodic patterns of electron densities at different altitudes of the ionosphere. The dominant diurnal and annual signals together with their Fourier series decompositions are obtained, which are consistent with the previous analyses on the total electron content. In the equatorial anomaly band, the annual component is weaker than its Fourier decomposition periods. In particular, the semiannual period dominates the annual component, indicating the relationship between the semiannual variation of the electron densities and the ionospheric equatorial anomaly. From detection of the phases of the components, it is revealed that the annual signal generally has its maximum value in summers at high altitudes, and in the winters at low altitudes. This is probably due to the higher [O/N₂] ratios in winter than in the summer in the lower ionosphere. Furthermore, the semiannual component mostly peaks around solstices or about a month before/after them.     

卫星产品多轴随机振动试验条件制定方法初探

卫星产品多轴随机振动试验技术的难点之一是试验条件的制定。文章分析了多轴随机振动试验条件制定的理论基础,并就多轴随机振动试验条件的工程处理方法从模型使用、简化处理、互谱设计、时域信号等4个方面进行了探讨,最后从简化处理、遥测数据分析、仿真计算和现有试验数据分析对比4个角度对卫星产品多轴随机振动试验条件的制定思路提出了建议。