电波极化面旋转特性研究

推导了电波极化面旋转角表达式, 利用实测电子浓度、地磁场磁感应强度模与磁倾角剖面,对定高载体、不同天线侧视方向与地球法线夹角、不同地区、不同频段、不同时段、不同太阳活动情况下的电波极化面旋转角进行了仿真, 并对仿真结果进行了分析, 得出了电波极化面旋转角的时域、地域、频域等规律和特性. 为这一领域的深入研究提供了参考.     

火星空间磁场结构特征

在火星空间模拟的单流体MHD模型的基础上, 研究了火星空间磁场结构及火星表面局部磁异常对磁场结构的影响. 在太阳风与火星相互作用的过程中, 形成弓激波和磁堆积区, 行星际磁场弯曲并向两极移动且被拖拽变形, 大部分磁力线从火星两极绕过, 通过火星之后在磁尾留下V字形结构. 火星表面附近局部磁异常也对火星磁场结构产生不可忽视的影响. 不同位置和强度的磁异常与太阳风相互作用形成结构及形态各异的微磁层, 如被拖拽的微磁层和存在开磁力线的微磁层等. 局部磁异常改变了近火磁场结构, 并可能改变等离子体的分布.     

三维流场的计算干涉方法

计算干涉技术通过试验图像和计算图像相比较，可以验证CFD的有效性，是研究复杂流场的有力工具。作者根据M-Z干涉仪的光学成像原理，用计算机仿真实现了将数值计算获得的二维、轴对称和三维的复杂流体的密度场转换为“无限条纹”和“有限条纹”的干涉图像，尤其是在处理三维流场时，采用流场重构的方法，达到了很好的效果。     

Velocity correlation functions of charged particles derived from the Fokker–Planck equation

An important ingredient in theories for diffusion of charged particles across a mean magnetic field are velocity correlation functions along and across that field. In the current article we present an analytical study of these functions by investigating the two-dimensional Fokker–Planck equation. We show that for an isotropic pitch-angle Fokker–Planck coefficient, the parallel velocity correlation function is an exponential function in agreement with the standard model used previously. For other forms of the pitch-angle diffusion coefficient, however, we find non-exponential forms. Also a new, velocity correlation function based, approach for deriving the so-called Earl-relation is presented. This new derivation is more systematic and simpler than previous derivations. We also discuss higher-order velocity correlations and the applicability of the quasi-normal hypothesis in particle diffusion theory. Furthermore, we compute velocity correlation functions across the mean field and develop an alternative theory for perpendicular diffusion.     

Optimal steering law of refractive sail

The interaction between electromagnetic waves and matter is the working principle of a photon-propelled spacecraft, which extracts momentum from the solar radiation to obtain a propulsive acceleration. An example is offered by solar sails, which use a thin membrane to reflect the impinging photons. The solar radiation momentum may actually be transferred to matter by means of various optical phenomena, such as absorption, emission, or refraction. This paper deals with the novel concept of a refractive sail, through which the Sun’s light is refracted by crossing a film made of polymeric micro-prisms. The main feature of a refractive sail is to give a large transverse component of thrust even when the sail nominal plane is orthogonal to the Sun-spacecraft line. Starting from the recent literature results, this paper proposes a semi-analytical thrust model that estimates the characteristics of the propulsive acceleration vector as a function of the sail attitude angles. Such a mathematical model is then used to analyze a simplified Earth-Mars and Earth-Venus interplanetary transfer within an optimal framework.     

Equilibrium positions on stationary orbits and planetary principal inertia axis orientations for the Solar System

We present a qualitative analysis in a phase space to determine the longitudinal equilibrium positions on the planetary stationary orbits by applying an analytical model that considers linear gravitational perturbations. We discuss how these longitudes are related with the orientation of the planetary principal inertia axes with respect to their Prime Meridians, and then we use this determination to derive their positions with respect to the International Celestial Reference Frame. Finally, a numerical analysis of the non-linear effects of the gravitational fields on the equilibrium point locations is developed and their correlation with gravity field anomalies shown.     

Progress in the Study of Galaxies: Structures,Collective Phenomena and Methods

The review contains the important achievements in dynamics of the galactic disks. Among them there are I. New structures discovered recently: • giant vortices (including giant anticyclone in the Solar vicinity); • slow bar; • inner oscillating structure within spiral arms similar that of enveloped soliton; • chaotic streamlines in the velocity field of the gaseous disk of a real galaxy. II. New collective phenomina discovered recently: • new overreflection instability initiating ‘mini-spiral’ in the innermost central parsec of Galaxy; • large-scale convection caused by nonlinear interaction of density wave with disk gas; • non-kolmogorovian spectrum of weak turbulence corresponding to the observed one in the • Solar vicinity. III. New methods worked out recently: • reconstruction of full three-dimensional vector field of gas velocity from the observed line-of- • sight velocity field; • observational test for verification of the wave-nature of the spiral arms; • observational test to distinguish two types of vertical motions: warp and z-motions in the • density wave; • derivation of correct system of two-dimensional dynamical equations from the initial three- • dimensional one. This revised version was published online in June 2006 with corrections to the Cover Date.     

冲击粗糙肋壁面流动特性实验研究

对有初始横流的冲击粗糙肋壁面的流场进行了流动特性实验研究 ,通过对大量实验数据的整理、分析以了解多种流动和几何参数对其流动特性的影响规律 ,为优化设计涡轮叶片内部冷却结构提供相应依据     

二元矢量喷管流场的N－S方程计算

对二元矢量喷管在不同工况下的流场进行了数值模拟。求解的控制方程为三维非定常Ｎ－Ｓ方程。空间方向用有限体积离散，时间方向用Ｒｕｎｇｅ－Ｋｕｔｔａ法推进。粘性项的计算上采用了一种有限体积框架下新的离散化方法。湍流模型采用了广泛使用的Ｂａｌｄｗｉｎ－Ｌｏｍａｘ代数模型。计算表明，本文方法能准确地计算二元矢量喷管、非矢量喷管在设计与大设计落压比下的流场。     

具有随机刚度薄板小挠度问题的数值分析

从薄板小挠度问题的控制方程出发,将结构的随机参数统一到刚度随机场中,采用局部平均法对刚度随机场进行离散,并将其融于二阶差分方法的列式中,给出了求解刚度随机时薄板上各点位移的数字特征的随机有限元法。该方法不但可以解决复杂边界下的薄板小挠度问题,而且进一步解决了结构的可靠度问题。文中最后对算例进行了计算,用解析解验证了本文方法的正确性。