树脂η*和Tg对C/E预浸料黏性的表征

针对复合材料预浸料工艺性缺少可量化表征方法的现状,研究了4种C/E预浸料的黏性及其环氧树脂体系的物理特性。发现预浸料黏性可以通过环氧树脂体系动态复数黏度η*和T_g两个物理量表征,环氧树脂的η*=35 kPa·s附近,T_g=0℃附近预浸料黏性较为合适。     

间断陡削化方法Ⅰ : 人为刚性源项方法——刚性常微分方程的计算方法的应用

本文针对界面运动的计算提出了适当附加人为刚性源项计算接触间断的方法。数值实验表明了这一方法是有效的。     

一种面向工程实际的专家系统的开发构思

面向应用领域中许多难度大，技术复杂的设计课题，本文探讨了专家知识的计算机程序系统。     

钱学森指导下的早期卫星准备工作

20世纪60年代初,四人小组在钱学森先生直接指导下为发展我国人造卫星进行早期准备工作。文章详细介绍了四人小组在钱学森先生指导下搜集学习国外有关卫星和空间技术的资料,编制《1964-1973年中国空间技术发展规划》（草案）,为大学生讲授星际航行概论课,以及担任星际航行座谈会秘书等工作。     

使用GAO-YONG模型对不可压圆管湍流的计算

基于有限体积法思想运用SIMPLER方法PLS格式求解轴对称柱坐标系下的GAO-YONG方程组,对管流边界层以及圆管湍流的自然转捩过程进行数值模拟。结果表明,方程不仅对于边界层流动的内层壁面律和外层亏损律能作出良好的预测,而且能够预报层流-湍流转捩过程中摩阻系数和速度型的变化。      

全光纤陀螺信号处理技术研究

采用数字、模拟混合信号处理方法，模拟信号处理主要针对光源驱动、相位调制器(PZT)的控制、相位跟踪、探测器信号的滤波和解调进行，数字信号处理器(DsP)根据模拟解调信号进行Sagnac相移计算、相敏参考信号自动选择，以及大小量程分档控制。此方法可有效发挥模拟、数字信号处理的优点，提高光纤陀螺的总体性能。     

Model of a fluxtube with a twisted magnetic field in the stratified solar atmosphere

We build a single vertical straight magnetic fluxtube spanning the solar photosphere and the transition region which does not expand with height. We assume that the fluxtube containing twisted magnetic fields is in magnetohydrostatic equilibrium within a realistic stratified atmosphere subject to solar gravity. Incorporating specific forms of current density and gas pressure in the Grad–Shafranov equation, we solve the magnetic flux function, and find it to be separable with a Coulomb wave function in radial direction while the vertical part of the solution decreases exponentially. We employ improved fluxtube boundary conditions and take a realistic ambient external pressure for the photosphere to transition region, to derive a family of solutions for reasonable values of the fluxtube radius and magnetic field strength at the base of the axis that are the free parameters in our model. We find that our model estimates are consistent with the magnetic field strength and the radii of Magnetic bright points (MBPs) as estimated from observations. We also derive thermodynamic quantities inside the fluxtube.     

“Biospherics” approach for studies of natural and artificial ecosystems

The main unifying feature of natural and artificial ecosystems is their biotic turnover (cycling) of substances which is induced with energy fluxes. A new integrating scientific discipline – Biospherics – studies biotic cycles (both in experiments and in mathematical models) of different degree of closure and complexity. By its origin, Biospherics is to be connected with extensive studies of Biosphere by Russian academician Vladimir Vernadsky. He developed and used “empirical generalizations” based on innumerous observations, comparisons and reflections. His “bio-geo-chemical principles” of Biosphere and ecosystems development have more qualitative than quantitative nature. Quantitative criteria to evaluate the efficiency of natural and artificial ecosystems are to take into account energy fluxes and their use in ecosystems of different types. At least, three of them are of value for estimation of natural and artificial ecosystems’ functional activities. Energy principle of extensive development (EPED), energy principle of intensive development (EPID) and main universal (generalized) criterion (MUC). The last criterion (Principle) characterizes the specific cycling rate of limiting chemical elements in multi-organism systems, developing under external energy fluxes. Its value can be a quantitative measure of effectiveness for every ecosystem functioning, including our global Biosphere. Different examples of these (above-mentioned) integrated criteria actions are presented and analyzed in the paper.     

Resonant motion, ballistic escape, and their applications in astrodynamics

A special set of solutions governing the motion of a particle, subject to the gravitational attractions of the Earth, the Moon, and, eventually, the Sun, is discussed in this paper. These solutions, called resonant orbits, correspond to a special motion where the particle is in resonance with the Moon. For a restricted set of initial conditions the particle performs a resonance transition in the vicinity of the Moon. In this paper, the nature of the resonance transition is investigated under the perspective of the dynamical system theory and the energy approach. In particular, using a new definition of weak stability boundary, we show that the resonance transition mechanism is strictly related to the concept of weak capture. This is shown through a carefully computed set of Poincaré surfaces, at different energy levels, on which both the weak stability boundary and the resonant orbits are represented. It is numerically demonstrated that resonance transitioning orbits pass through the weak stability boundaries. In the second part of the paper the solar perturbation is taken into account, and the motion of the resonant orbits is studied within a four-body dynamics. We show that, for a wide class of initial conditions, the particle escapes from the Earth–Moon system and targets an heliocentric orbit. This is a free ejection called a ballistic escape. Astrodynamical applications are discussed.