多Agent智能制造系统研究综述

Agent与多Agent系统是分布式人工智能的主要研究方向之一，Agent技术已经被认为是进行分布式工业系统建模的一种重要方法，是设计与实施分布式智能制造环境的最自然的手段，是构建下一代制造系统的重要技术之一，基于Agent的制造系统是多Agent系统理论和方法在制造领域中的具体应用，在对Agent与多Agent系统技术研究进行简要总结的基础上，综述了Agent技术在制造企业集成，供应链管理、制造规划、调度和制造控制等方面的应用及其研究现状，并对Agent制造系统研究的主要内容及关键问题进行了探讨。     

IBM3880,3803在两台IBM4341主机中的共享

IBM3880是磁盘存贮控制器,IBM3803是磁带控制器。本文介绍了3880,3803作为两台IBM 4341主机共享外设的意义,分析讨论了这两种设备的结构原理及共享实现方法。     

Influence and optimization of parameters of prepreg viscosity during placement

This paper tested the viscosity of prepreg in the automatic placement process, and conducted the probe and placement-90° peel tests through the test systems. The law of variation of prepreg viscosity during the laying process was studied through these tests under different conditions by taking the peel force to intuitively and quantitatively characterise the viscosity of the prepreg.The results show that this viscosity is inversely proportional to the laying rate, proportional to the laying pres...     

On the optical variability of a be star,HDE 245770, — the optical counterpart of the transient X-ray pulsar A0535+26

Photoelectric WBVR observations of Be star HDE 245770=V 725 Tau, the optical counterpart of the transient X-ray pulsar A0535+26, having a pulse period of about 104 s, were conducted for more than 10 years. An irregular long-term optical variability of the star with amplitudes of the order of a few tenths of magnitude was found to be a usual phenomenon. In some cases rapid changes of the star's optical luminosity with a characteristic period of a few tens of minutes or a few hours, and an amplitude of several hundredths of magnitude in all the spectral bands used, which have practically coincided or correlated with the X-ray pulsar outbursts detected by X-ray satellites, were observed.Photoelectric recording of the optical flux from HDE 245770 were made in 1981–1982 with a time resolution of 1 second and 10 s, respectively, in theR spectral band (₀ 7000 Å) and in the narrowH -emission-line band (_1/2 75 Å) using a 48-cm reflector of High-Mountain Tien-Shan observatory of the Sternberg Astronomical Institute near Alma-Ata. An analysis of autocorrelation functions of the flux changes from object under study and a comparison with the star BD+26° 876 indicated the variability of luminosity of V 725 Tau in theR spectral band on a time scale of a few tens of second; this variability resembles shot noise with a characteristic time of stochastic bursts of about 15–20 s and their amplitudes of about a few tenths of a percent. InH -emission-line radiation autocorrelation functions and power spectra show quasiperiodic variability of luminosity of HDE 245770 with a characteristic period of about 100–150 s and an amplitude in the neighbour-hood of 0.5%. The latter result is not quite reliable because of not quite fine weather conditions during the observations; independent observations and check-up are required.     

仿射非线性系统鲁棒干扰解耦问题可允许摄动范围的研究

对于仿射非线性系统，本文研究了在系统存在不确定时，鲁棒干扰解耦问题。给出了干扰可测和不可测两种情况下，保持标称系统干扰解耦性质不变的可允许摄动范围。     

方块脉冲函数应用于线性时变系统最优控制的动态规划解法及其改进

本将方块脉冲函数应用于线性时变系统最优控制问题。首先将该问题转化成多段动态规划表示形成，通过求解多段动态规划问题，可得原问题的分段常值解。进而，根据最优控制的存在条件下及对边界条件的进一步处理，导出了原问题更为简明的动态规划表示，使求解结果更为简洁，明潦。与献（１），（２），（３）中的求解方法比较，得到的递推算法简单，便于计算机求解，且不必求解ｍ个２ｎ×２ｎ阶逆矩阵，使计算量及存贮空间大为减少     

空间可展开天线结构研究进展

扼要综述了空间可展开天线结构的发展及目前的国际动态,叙述了空间可展开天线结构、设计及分析中的主要研究课题及其目前的进展。指出“把多体动力学与有限元法相结合的综合动力学建模法”、“辩识模型后,用预测控制和优化的思想进行展开过程控制”、“用多约束优化法调整网状天线反射面形状精度”等是适合我国目前状况的较好方法。     

非线性系统的可控正则型和状态变换的求法

Zeitz引入了非线性控制系统的可控正则型,证明了由可控正则型描述的非线性系统是可控的,本文进一步给出了非线性系统正则化的条件和状态变换的算法,从而解决了通过状态变换证明非线性系统的可控性。     

开环全保偏光纤陀螺研究

开环全保偏光纤陀螺结构简单，有使用价值；进入９０年代国外研究成功熔接型保偏光纤耦合器以后，这种陀螺更受重视，向实用方向发展，对研究全保偏光纤陀螺中的几个关键问题，光路中元器件的特性；保偏光纤的对轴熔接技术，零漂和噪声做了分析，实验结果表明，零漂达到１．２４°／ｈ。