关于Davidson—Lanczos方法的收敛率

本文对文[1]提出的求解大型对称矩阵A的极端(几个最大或最小)特征值及相应特征向量的Davidson—Lanczos方法,用Rayleigh—Ritz逼近理论,研究了该方法的收敛率。证明了由该方法产生的规范正交向量{v_i}_i~m=1是Krylov子空间K_m≡Span(v_1,Av_1,…,A~(m-1)v_1)的一组基。设A的k个最大特征值为又,λ_1>λ_2>…>λ_k,相应的近似特征值为λ_i~(m)(i=1,…,k),得到 这里γ_i(γ_i>1),W_i和W_i~(m)是常数。     

平面超椭圆曲线的二次NURBS逼近

基于超椭圆曲线的基本性质、方程及其图形表示,研究了超椭圆曲线指数s和欲逼近的二次NURBS曲线权重系数w之间的对应关系,给出了超椭圆曲线的一种高精确的二次NURBS逼近方法,避免了因超椭圆曲线取点误差而可能产生的对生成曲面的影响,也大大缩减了计算量。文中给出了超椭圆曲线的二次NURBS逼近效果图,探讨了将此方法用于飞机机身曲面外形设计的相关步骤。     

考虑粘性时激波反射及壁面热流计算

本文采用显式 TVD 格式,求解薄层 Navier-Stokes 方程,计算了激波与楔面相互干扰的流场情况,得出了马赫反射的各种等强度线及固壁面上详细的物理量分布,根据计算得出的流场,计算了壁面摩擦阻力及热流分布。     

Families of halo orbits in the elliptic restricted three-body problem for a solar sail with reflectivity control devices

Solar sail halo orbits designed in the Sun-Earth circular restricted three-body problem (CR3BP) provide inefficient reference orbits for station-keeping since the disturbance due to the eccentricity of the Earth’s orbit has to be compensated for. This paper presents a strategy to compute families of halo orbits around the collinear artificial equilibrium points in the Sun-Earth elliptic restricted three-body problem (ER3BP) for a solar sail with reflectivity control devices (RCDs). In this non-autonomous model, periodic halo orbits only exist when their periods are equal to integer multiples of one year. Here multi-revolution halo orbits with periods equal to integer multiples of one year are constructed in the CR3BP and then used as seeds to numerically continue the halo orbits in the ER3BP. The linear stability of the orbits is analyzed which shows that the in-plane motion is unstable while the out-of-plane motion is neutrally stable and a bifurcation is identified. Finally, station-keeping is performed which shows that a reference orbit designed in the ER3BP is significantly more efficient than that designed in the CR3BP, while the addition of RCDs improve station-keeping performance and robustness to uncertainty in the sail lightness number.     

A novel surrogate modeling strategy of the mechanical properties of 3D braided composites

In this paper, a surrogate-based modeling methodology is developed and presented to predict the elastic properties of three dimensional (3D) four-directional braided composites. Using this approach, the prediction process becomes feasible with only a limited number of training points. The surrogate models constructed using Finite Element (FE) method and Diffuse Approximation, reduce the computational time and cost for preparing experimental samples. In the FE model, multiscale method is applied to couple the computations of elastic properties at microscale and mesoscale. Subsequently, a parametric study is performed to analyze the effects of the three design parameters on the elastic properties. Satisfactory results are obtained via the surrogate-based modeling predictions, which are compared with the experimental measurements. Moreover, the predictions obtained from surrogate models concur well with the FE predictions. This study orients a new direction for predicting the mechanical properties based on surrogate models which can effectively reduce the sample preparation cost and computational efforts.     

宏指令在变螺距螺旋轨迹编程中的应用

以一个现实的零件,表述了宏指令在变螺距螺旋加工中的运用,利用函数的合成,循环语句的运用,细致而详细地描述了程序编制的整个过程。对于复杂空间曲线,若能建立函数的关系,通过宏指令的运用,也能手动编制出简洁的复杂轨迹,且应用面广,程序段直观而清晰,更具可读性。     

DE历表的结构、计算与比较

在详细介绍美国JPL(Jet Propulsion Laboratory,喷气推进实验室)发布的DE (Development Ephemerides,行星/月球展开历表)系列历表的基本情况、头文件和数据文件的结构、历表计算原理等内容的基础上,以DE405、DE421、DE431为例,分别计算了1900-2200年间月球、太阳、行星等天体在地心天球参考系中的坐标及速度,并由此得到3个历表间的差异,结果表明DE431与DE421之间的差异,整体而言要小于二者同DE405之间的差异.最后以引潮力的计算为例,表明历袁更新对于引潮力的影响基本可忽略不计,验证了IERS(International Earth Rotation and reference systems Service,国际地球自转与参考系服务)规范中关于历表更新对相关地球科学影响十分有限的结论.     

水凝物对THz波辐射的衰减研究

文章基于水凝物粒子尺寸与THz波长的大小关系,分别利用Rayleigh近似、Mie理论以及几何光学方法计算了降雨和云雾引起THz波辐射的散射衰减。比较了不同强度的降雨和不同能见度、含水量的云雾对THz波的散射衰减。结果表明,随着频率的增大,THz波段雨衰减先增大后减小;在整个THz波段,含水量较小或能见度较低的云雾的衰减随频率的增大而单调增加,含水量较大或能见度较大的云雾的衰减随频率先增大后减小;在THz波段云雾衰减随能见度的减小和含水量的增加而增大,温度对THz波段的云雾衰减影响不大,在整个THz波段并不存在明显的规律。在THz波频率高端云雾影响较降雨要严重的多。     

矩阵方程A×B=C的中心对称解

文章研究了矩阵方程的中心对称解.利用矩阵对的广义奇异值分解给出了该方程有中心对称解的充分必要条件,以及解的通式,证明了最佳逼近问题存在唯一解,并给出了求最佳逼近解的算法和数值箅例.     

特征值反问题逼近解与极值化解的统一应用

基于矩阵最佳逼近与加权残值理论,本文把求解特征值反问题的矩阵逼近法和极值化方法统一为不同范数定义下的最小二乘问题。这对解决部分特征值和／或特征向量给足情况下的反问题提供了一个有效工具。结合工程实际,本文给出了具体应用的数值例子。