复合材料桁架式发动机支架改型设计分析

采用DFH-3改进型平台的卫星变轨发动机支架直接安装在承力筒下锥段的内壁,要求在正弦振动载荷条件下,变轨发动机安装法兰面的最大加速度响应(5Hz~100Hz范围内)不得超过3g。针对上述条件,本文对DFH-3改进型平台变轨发动机支架直接继承现有产品的可行性进行了分析,并对几种可能的设计变更方式进行了分析,最终得到了对变轨发动机支架结构进行加强的优选方案。     

改进格网型中的跨音速分析和设计计算

 <正> 近年来采用不同的主控方程计算跨音速绕流的方法有了不断的发展和改进,越来越多的算例表明了计算流体力学的迅速发展,其中解全速势方程的跨音速计算方法也有了很大进展,并已为国外航空工业界广泛地应用于设计和分析计算中。其中有限体积方法提高了处理复杂外形的能力,若采用多重网格技术则可改进计算效率。但是为了发展一种普遍适用和可靠的格网系统以耦合有限体积算法仍有许多工作要做     

平面度误差目标函数凸凹性的研究

证明了平面度误差最小区域评定法的目标函数是二维欧氏空间R2 中的连续、不可微的凸函数 ,从而证明了目标函数的全局极小值是唯一的。     

SPACE LIFE SCIENCE IN 2000-2001

Chinese scientists studied some of the problems in the field of space life science and achieved success in the area during 2000-2001. Space biological experi ments were carried out in the orbit and the results of ground studies on protein crystallization, space radiation, space motion sickness were introduced in this paper. The influences of simulated weightlessness on the brain-function, the car diovascular, endocrine hormones, immunity, skeletal and muscle systems were presented. In addition, gravity medicine and space environment medicine, as well as countermeasures to space deconditioning, such as the traditional Chinese medicine, were also reported.     

沃尔什函数理论中并元移位概念的物理解释

并元移位的概念在沃尔什函数的理论中有着重要的作用,但是,至今为止,未见有人对它的物理意义做出合理的解释.从复制理论的角度出发,在简要介绍复制理论的基础上,通过研究复制序列的位置相关性,揭示了并元移位实际上是一种特殊的距离定义,从而较为深刻地解释了并元移位概念的物理意义.     

关于非结构网格生成中的背景函数

背景信息对于用阵面推进法生成非结构网格是一个关键的环节.文章基于众多文献中提到的背景信息提供方法,提出一种更为实用的背景信息提供技术.此方法不仅避免了不必要的机时,内存的消耗,又使网格具有光滑性,网格的生成具有灵活性,方便性的特点.基于生成的网格采用有限体积法研究无粘高超音速化学非平衡流的流场分布,生成的网格能够成功的运用于高超音速化学非平衡流的数值计算。     

热障涂层红外热无损检测的建模和有限元分析

在柱坐标系下以轴对称模型描述热障涂层结构TNDT(Thermal Non-Destructive Testing)的瞬态热传导,建立相应的物理模型.用有限元分析软件ANSYS计算热障涂层结构受热脉冲激励后的温度场,研究TNDT可检信息参数(如最大温差和最大对比度)与脱粘缺陷半径、深度、涂层厚度的关系.结果表明,在涂层厚度一定时,最大温差和最大对比度与脱粘缺陷半径成非线性关系,它们随着缺陷半径的增大而增加,且存在上限饱和值;在缺陷半径一定时,最大温差和最大对比度与涂层厚度成非线性关系,且随着涂层厚度的增加而减小.这些研究结果为热障涂层内部脱粘的红外热无损检测及表征提供了基本理论依据.     

铝试件脉冲红外热无损检测的主分量分析

为了提高铝试件脉冲红外热像无损检测的缺陷探测能力,研究了主分量分析法在热像信号处理中的运用方法及效果.结合脉冲热像序列处理论述了主分量分析的数据准备、计算方法和处理效果.为了考查算法的有效性,对铝合金板进行了脉冲红外热像无损检测实验.结果表明,采用第2、第3主分量图像以及由前几个主分量重建的图像均有增强缺陷对比度和抑制加热不均的效应,从而提高了脉冲红外热无损检测的缺陷检测能力;此外,在检测铝板模拟腐蚀时,能使可探测的最小腐蚀率减小10%左右.     

Using the radial basis function neural network to predict ionospheric critical frequency of F2 layer over Wuhan

Neural networks (NNs) have been applied to ionospheric predictions recently. This paper uses radial basis function neural network (RBF-NN) to forecast hourly values of the ionospheric F₂ layer critical frequency(f_oF₂), over Wuhan (30.5N, 114.3E), China. The false nearest neighbor method is used to determine the embedding dimension, and the principal component analysis (PCA) is used to reduce noise and dimension. The whole study is based on a sample of about 26,000 observations of f_oF₂ with 1-h time resolution, derived during the period from January 1981 to December 1983. The performance of RBF-NN is estimated by calculating the normalized root-mean-squared (NRMSE) error, and its results show that short-term predictions of f_oF₂ are improved.     

Improved interpretation of solar wind ion measurements via high-resolution magnetic field data

The Wind   spacecraft’s Faraday cups (FC) continue to produce high-quality, in situ observations of thermal protons (i.e., ionized hydrogen) and α$\alpha$-particles (i.e., fully ionized helium) in the solar wind. By fitting a Wind/FC ion spectrum with a model velocity distribution function (VDF) for each particle species, values for density, bulk velocity, and temperature can be inferred. Incorporating measurements of the background magnetic field from the Wind Magnetic Field Investigation (MFI) allows perpendicular and parallel temperature components to be separated. Prior implementations of this analysis averaged the higher-cadence Wind/MFI measurements to match that of the Wind/FC ion spectra. However, this article summarizes recent and extensive revisions to the analysis software that, among other things, eliminate such averaging and thereby account for variations in the direction of the magnetic field over the time taken to measure the ions. A statistical comparison reveals that the old version consistently underestimates the temperature anisotropy of ion VDF’s: averaging over fluctuations in the magnetic field essentially blurs the perpendicular and parallel temperature components, which makes the plasma seem artificially more isotropic. The new version not only provides a more accurate dataset of ion parameters (which is well suited to the study of microkinetic phenomena), it also demonstrates a novel technique for jointly processing particle and field data. Such methods are crucial to heliophysics as wave-particle interactions are increasingly seen as playing an important role in the dynamics of the solar wind and similar space plasmas.