铁磁性纳米线阵列的偏差对磁性的影响

用蒙特卡洛方法对纳米线阵列磁滞回线进行模拟,研究了纳米线排列、长度和直径的偏差对纳米线阵列整体磁学性质的影响。研究结果表明,纳米线位置的标准偏差引起了矫顽力和磁化率降低;长度的标准偏差则仅仅引起饱和磁化强度的增大和剩余磁化强度的减小,而对矫顽力没有影响;直径的的标准偏差对纳米线阵列产生了比较复杂的影响。     

A robust solution for hesitate phenomenon in pick up process of aerospace electromagnetic relay

As for aerospace electromagnetic relay (AEMR) which is of small batches and having difficulty in automatic production, the uncertainty phenomenon is remarkable due to excessive manual work involved in the assembly and adjustment processes. This kind of uncertainty may increase the coil voltage difference (CVD) caused by hesitate phenomenon in the pick up process of AEMR. Taking a certain type of AEMR for example, the CVD problem in the actual producing process has been studied in this paper. The primary cause of this issue, two-steps of armature motion (namely hesitate phenomenon) in the pick up process, has been found by analyzing the matching characteristics of electromagnetic and mechanical torques of AEMR. Through the optimization of the matching characteristics, the two-steps of armature motion problem is solved by robust design of the return reed which is a key part of AEMR. The validity of this research has been proved by the comparison of characteristics of AMER before and after the optimization.     

圆弧型线指尖密封结构的形成方法和迟滞性能分析

对圆弧型线指尖密封结构的形成方式进行了分析和研究,在此基础上采用有限元技术对圆弧型线指尖密封结构的迟滞性能进行了计算分析。计算结果表明:在相同的展开角范围内,2种圆弧型线指尖密封结构的迟滞性能要优于对数螺线指尖密封结构的迟滞性能,圆弧型线弧长较短的指尖密封结构的迟滞性表现更优。     

迟滞非线性系统的建模与控制研究综述

研究了迟滞非线性系统研究的发展历程,归纳了迟滞非线性系统在建模和控制方面的国内外研究现状,以及在高精度控制平台、声纳系统和智能材料和结构上的应用,并对迟滞非线性系统建模与控制的未来发展方向进行了展望。     

基于DSP的并联型有源电力滤波器控制方法的研究

通过对滞环PWM技术和三角波PWM技术的分析和研究,以及跟踪电流和输出电流之间的关系,提出了一种改进的有源电力滤波器的控制方法。在以DSP为核心控制器的基础上,对其进行了实验研究,并对试验的结果进行了分析。试验结果说明这种控制方法控制的SAPF具有实时性好,误差小,系统运行稳定的特点。     

The structure of the solar cycle maximum phase in the galactic cosmic ray 11-year variation

Two phenomena connected with the maximum phase of the 11-year solar cycle in the galactic cosmic ray intensity – the change in the energy dependence of the intensity variations and the double-peak structure in the intensity modulation time profile – are considered for the last five solar cycles (Nos. 19–23). The distinct 22-year cycle in the magnitude of the so called energy hysteresis is observed.The periods of the solar cycle maximum phase in the galactic cosmic ray intensity, characterized by the specific energy dependence of the intensity, are estimated. It is found that the double-peak structures belonging to the solar cycle maximum phase and those around it are very similar both in the amplitude and in its energy dependence.     

各种排列双圆柱绕流相干性研究

本文讨论了各种排列双柱绕流的相干性问题。低湍流度高Re数的实验表明升力是由尾涡诱导引起的,而双稳态现象是由尾涡不稳定性引起的。此外,还对高湍流度状态作了探索性的工作,发现由于尾涡的可分性和狭缝流方向的不稳定性所共同引起的双稳态现象与低湍流度的情况有很大不同,升力和阻力也是如此。     

塑性变形提高形状记忆合金相变滞后机制的探讨

形状记忆合金经适当温度下的塑性变形可以有效地提高马氏体的稳定性,从而使相变滞后得以大幅度提高.本文根据马氏体相变热力学和动力学,并结合相关的实验结果,研究了弹性应变能弛豫和相变滞后的关系.结果表明,塑性变形产生的位错以及变形的第二相颗粒对逆马氏体相变温度的提高具有一定作用,但塑性变形导致应变能释放才是形变提高形状记忆合金相变滞后的主导因素.     

应变反馈式压电陶瓷微位移驱动器的研制

介绍了采用应变片测量压电陶瓷微位移驱动器位移的原理和设计思想，介绍了实验装置的结构，给出了实验结果，证明将应变片直接粘贴在压电陶瓷基体表面测量其位移的方法是可行性的；通过对压电陶瓷滞回特性的测定，提出了建立压电陶瓷的控制模型的基本思路。     

迟滞非线性气动弹性反馈线性化自适应控制

首先将含操纵面二元机翼的动态方程以状态空间形式描述,基于Lie导数对其进行了输入/输出局部反馈线性化;然后考虑迟滞非线性模型存在参数不确定性的情况下,利用Lyapunov稳定性理论进行了自适应控制律设计.仿真结果显示:在内动态稳定的情况下,所设计的控制律能够使开环不稳定气动弹性系统受扰后快速地回复到原来的稳定状态,并且在控制面偏转存在限制的情况下仍能实现对非线性颤振的控制.