二维计算机图象检测系统

目前,利用机器视觉系统监测生产过程和进行质量控制是一个非常活跃的研究领域。当把视觉系统用于几何量测量时,必须解决其硬件的分辨力极限所带来的问题:测量精度高意味着测量范围小,或者,测量范围大意味着测量精度低。提出了解决上述问题的方法:一个由步进电机驱动的XY工作台与图象处理系统相结合。产生出一个多坐标系统结构。测量参数在两个坐标系之间传送,并在100mm×100mm范围内,在X和Y两个方向,达到的测量精度为0.02mm。     

Transition radio emission of mildly relativistic particles

We report new calculations of transition radiation spectra which are correct for arbitrary energy of a particle at all frequencies down to plasma frequency. The importance of the emission mechanism for solar flares are discussed.     

W33A的羟基分子脉泽辐射

本文给出了Ｗ３３Ａ在两个跃迁频率上的左右图偏振ＯＨ脉泽辐射谱线，采用细管和球模型，获得脉泽活动区的氢分子数密度近似１０７ｃｍ３．为了获得１０４６ｓ１量级脉泽光子发射率，两种模型一致要求抽运率为１（ＯＨ）ｃｍ３ｓ１，但球型脉泽活动区要求较高的抽运效率．     

8802超低频标准相位产生器

８８０２超低频标准相位产生器采用数字技术，用Ｄ／Ａ变换方法产生正弦信号，由单片机控制频率和相位，频率由晶振综合产生，相位可数字预置，频率准确度高至±５×１０￣（－６），相位准确度高至±０．０００２°。介绍了主要技术指标、工作原理、技术特点和误差分析等。     

建立虚拟现实空间的好助手-VRML

介绍了虚拟现实技术及VRML虚拟现实建模语言的概念,提出了用VRML虚拟现实建模语言设计软件时应该注意的一些问题,说明了用VRML虚拟现实建模语言设计的软件适用的范围,探讨了解决虚拟现实技术中存在问题的方法.     

计算机翼跨声速绕流的全速位积分方程数值解

本文利用格林定理将全速位方程转换为全速位积分方程，应用高斯定理对沿激波面的显式积分进行简化。将全速位积分方程的解表示成为面元项和场元项之和，然后离散进行数值求解。本文将激波捕捉方法和激波装配技术结合起来，对机翼跨声速绕流进行数值实验，计算结果令人满意。     

Infrared spectrometer PFS for the Mars 94 orbiter

Thin films containing a mixture of aliphatic (glycine) and aromatic (tryptophan or tyrosine) amino acids were exposed to a vacuum ultraviolet radiation (VUV) with wavelenghts 100–200 nm. Dipeptides (glycyl-tryptophan and glycyl-tyrosine) were synthesized in these conditions. We compared the actions of VUV and γ-radiation. Polymerization is an essential step in prebiological evolution and we have shown that this stage probably occured over an early Solar system history.     

小型弹体转动惯量的测定

阐述了对称式三线摆的结构原理及该摆微角与大角摆动周期的计算方法 ,利用此摆可以测量构件的转动惯量。当 RL <130 、φ0 <6 0°时 ,该装置的测量准确度优于 1%。     

On the mechanisms of cooling of the nightside thermosphere of venus

The plausible mechanisms of cooling of the nightside Venus' thermosphere are analysed with the aid of the model of the atmospheric heat budget that incorporates, in addition to thermal conduction and IR radiation in the 15 μ band of CO₂, heating and cooling due to global scale winds, eddy turbulence, and IR radiation in the rotational bands of H₂O and CO, as well as the 63 μ line of atomic oxygen. The H₂O mixing ratio and parameters of turbulence required for cooling of the thermosphere down to the observed low temperatures are evaluated.