Surface tension-driven flows in horizontal liquid metal layers

The problem of surface tension-driven flows in horizontal liquid layers has been studied experimentally, and theoretically by direct numerical simulation and small perturbation analysis. We focus our attention on situations in which the depth of the fluid (liquid tin; small Prandtl number, Pr=0.015) is small enough to ensure the predominance of the surface tension forces over those due to the buoyancy. The surface velocity has been experimentally obtained for liquid tin layer with various aspect ratio (length to height) in the range 5<A<83. The thermal gradients are ranged from 5 to 40°K/cm. In the numerical study, the Navier-Stokes and energy equations are solved by an efficient finite difference technique. The parameters governing the flow behaviour in the liquid are varied to determine their effects on thermocapillary convection: the Reynolds number 10<Re<210⁴ and the aspect ratio 2<A<25; with Pr kept constant at Pr=0.015. The linear eigenequation resulting from small spatial disturbances of the Couette flow solution is solved using an Tau-Chebyshev approximation. A notable feature of the theoretical study is the totally different end circulations. In the region near the cold wall a multicell structure is evident. This agrees with the eigensolution which is of complex type, indicating spatial periodicity. In the hot wall region the flow is accelerated to reach the velocity value for the fully-developed Couette flow which is reached under conditions such as Re/A<20. The transition from viscous to boundary layer regime occurs for a critical value (Re/A)_c of nearly about 200, as deduced from the numerical and experimental results.     

CPL蒸发器传热和蒸发流动过程的分布参数模型

针对ＣＰＬ蒸发器，建立了可据以分析其传热过程和蒸发流动过程的分布参数模型，并就一个模拟算例进行了考察，得出了有意义的结论。该模型较之传统集中参数模型的优点在于，其计算结果反映出了蒸发器内沿轴向流动过程中各肋壁温度及肋壁与流动工质之间换热系数大小的变化情况以及蒸发器内局部蒸汽（或液体）的热力状况，因而为从细节上揭示ＣＰＬ蒸发器的传热性能及其工程模型的试验研究、优化设计等打下了一定的基础     

INS／GPS组合导航系统的容错研究

本文研究了INS/GPS组合导航系统的容错问题,并提出了一个两级故障检测及分离方案。通过采用该方案,INS/GPS组合导航系统将具有较高的容错能力,并能为用户提供连续、精确的导航信息。     

Some comparisons of orbit determination and parameter estimation based on LAGEOS 1 and LAGEOS 2 data

The modelling accuracy of the LAGEOS 1 orbit was continously improved since its launch in 1976. In spite of these experiences the modelling accuracy of LAGEOS 2 is still about 20 per cent worse. Considering e. g. only the influence of different gravity field models it has been shown that the orbital fits for arc lengths of one month is generally about 25 mm for LAGEOS 1 and more than 30 mm for LAGEOS 2. This is mainly due to the fact that LAGEOS 2 has not yet been used for the determination of most gravity field models. The influences of different model parameters on the estimation of station coordinates, Earth rotation parameters, the geogravitational coefficient, the radiation pressure coefficient, and the empirical acceleration has been studied. The differences and peculiarities of both satellites are discussed. Although the analysis of LAGEOS 2 data still does not reach the high level of LAGEOS 1 combination solutions using both satellites allow new insights, higher accuracies, and a higher time resolution for the parameters and phenomena investigated.     

Formation of amino acid precursors in cometary ice environments by cosmic radiation.

Cometary ices are believed to contain water, carbon monoxide, methane and ammonia, and are possible sites for the formation and preservation of organic compounds relating to the origin of life. Cosmic rays, together with ultraviolet light, are among the most effective energy sources for the formation of organic compounds in space. In order to study the possibility of the formation of amino acids in comets or their precursory bodies (interstellar dust grains), several types of ice mixtures made in a cryostat at 10 K ("simulated cometary ices") were irradiated with high energy protons. After irradiation, the volatile products were analyzed with a quadrupole mass spectrometer, while temperature of the cryostat was raised to room temperature. The non-volatile products remaining in the cryostat at room temperature were collected with water. They were acid-hydrolyzed, and analyzed by ion-exchange chromatography. When an ice mixture of carbon monoxide (or methane), ammonia and water was irradiated, some hydrocarbons were formed, and amino acids such as glycine and alanine were detected in the hydrolyzate. These results suggest the possible formation of "amino acid precursors" (compounds yielding amino acids after hydrolysis) in interstellar dust grains by cosmic radiation. We previously reported that amino acid precursors were formed when simulated primitive planetary atmospheres were irradiated with cosmic ray particles. It will be of great interest to compare the amount of bioorganic compounds that were formed in the primitive earth and that brought by comets to the earth.     

等厚度楔形杆的应力分析

本文将应力场分为基本应力场和修正应力场两个部分。基本应力场的应力σ_x用勒让德级数展开,级数的前两项系数用截面法确定;其他应力τ_(xy),σ_y由平衡方程和侧表面边界条件确定;再用余能原理确定其余各项系数。由于该级数收敛很快,故可得到封闭解并能给出该解的应用范围,为精确满足自由端的静力边界条件,又引入一个从自由端到固定端迅速衰减的修正应力场,该应力场的应力在自由端等于已知外力与基本应力解之差。其确定方法与基本应力场相同,它也有一个封闭解。将以上两应力场相加卽可得到满足全部边界条件的解。     

四足步行机运动机构及步态参数对行走稳定性影响分析

本文研究了四足步行机的行走稳定性问题,建立了考虑运动机构包括腿机构及其传动系统影响的稳定性模型;分析了各步态参数对稳定性的影响,并以研制的四足步行样机为例进行了计算机仿真。     

1989年3月太阳活动引起的强烈磁暴群

本文分析了1989年3月上旬一个太阳超级活动区中多次特大耀斑引起的强磁暴群.联系源耀斑的等级、位置等讨论了磁暴形态特征.随着耀斑活动区位置由东向西旋转,磁暴的形态呈现有规律的变化,充分显示了磁暴形态特征有依赖于耀斑位置的中心子午线效应和东西不对称性.     

随机多变量连续系统的辨识

本文讨论了由随机向量微分方程描述的多变量连续系统的辨识问题。虽然假定微分方程中的噪声项是白噪声,但是用方脉冲函数积分微分方程后,所得到的代数方程中的噪声项却是有色噪声。为了得到无偏的参数估计,本文提出一种预滤波方法。仿真例子表明这种方法是很有效的。     

毛细泵环中两相循环回路的初步分析研究

本文初步分析研究了在微重力或失重情况下毛细泵环中两相循环回路的稳态流动，情况，提出了基于力平衡的两相循环回路一维稳态数学描述。从计算结果得出了最佳有效毛细孔半径等结论。