电动机器人脉宽调速系统的研制

本文介绍用于DGR-5A五自由度电动机器人关节伺服回路的脉宽调速系统。主要介绍脉宽调制型功率放大的工作原理及设计方法,同时简要介绍关节伺服回路的设计。     

帆板控制系统设计

该帆板控制系统采用塑料薄膜电位器作为传感器检测角度信号,检测到的角度信号经信号处理电路送12位的串行接口A/D转换器ADS7818进行数字化转换,转化结果由Cortex-M3处理器LM3S615进行处理产生PWM控制信号,该控制信号经功率VMOS驱动电路实现轴流电扇的速度调节,从而实现帆板角度定位闭环控制。通过按键可以实现帆板角度的设定及运行控制,设置六位LED数码管显示实现角度及其它运行状态的显示。经过实际测试该系统完全达到了设计要求的各项指标要求。     

一种数字调制方式自动识别算法

介绍了利用6个特征参数对7种数字调制方式进行调制方式的自动识别模型算法及仿真结果,表明所提出的自动识别算法能够很好的识别出各种数字调制信号,同时具备算法简单、速度快和准确率高的优点。     

煤油/空气脉冲爆震发动机强化燃烧装置

为了研究不同结构强化燃烧装置对煤油/空气混合物爆震起爆过程的影响, 选择适应于煤油/空气气动阀式脉冲爆震发动机使用的强化燃烧装置, 设计加工了几种不同结构的强化燃烧装置, 在内径100mm的爆震管内进行大量爆震试验.分析了不同结构强化燃烧装置的工作机理, 比较了不同强化燃烧装置对煤油/空气混合物爆震起爆过程的影响.研究结果为优化设计强化燃烧装置, 优化设计煤油/空气气动阀式脉冲爆震发动机原理样机提供了初步理论基础.      

一种抑制控制力矩陀螺框架电机共模电压的方法

控制力矩陀螺作为执行机构,是保障航天器在轨寿命和工作性能的核心部件之一。为了抑制控制力矩陀螺外框电机的共模电压,提高控制力矩陀螺的在轨寿命,本文提出了一种三相四桥臂的拓扑结构与优化的SVPWM调制算法结合的共模电压抑制方法,调制过程中避免零矢量的使用,使驱动器可以保持在平衡状态,经过仿真试验的结果对比分析,验证了这种方法可以有效的抑制系统的共模电压。     

一种地球同步自旋卫星红外弦宽差分定姿方法

 提出了一种定点后地球同步自旋卫星姿态确定方法,推导了它的计算公式。充分利用了定点后卫星相对地球位置固定不变的特点,只利用一个参考矢量和卫星的位置信息,就可以确定卫星的姿态,完全消除了传统定姿态方法的几何条件限制。由于本方法姿态计算过程中利用的是星上红外地球敏感器测量数据的差分值,消除了测量数据中系统差对定姿精度的影响,使定姿精度提高到0.01°,实际工程应用效果进一步证明了该算法的正确性和精度。     

噪声调幅干扰信号波达方向估计研究

利用噪声调幅干扰信号频谱结构的特殊性,提出基于阵列接收信号载频处频域数据的波达方向估计算法,通过仿真分析表明该算法的角度估计性能明显高于目前广泛采用的比幅比相单脉冲测角法,并且计算量也大大低于传统的波达方向估计算法.     

卫星遥测功率谱分析和调制度测量方法研究

残余载波调制是卫星测控中的常用调制体制。文章从理论上给出了该体制下信号的功率谱密度表达式,得到奇次谐波谱线展宽等结论,并通过仿真和实验进行了验证。利用所得结论讨论了遥测调制度测量方法,提出通过功率谱的2阶边带进行测量可以使结果得到改善。     

Sunspot activity and cosmic ray modulation at 1 a.u. for 1900–2013

The descent of sunspot cycle 23 to an unprecedented minimum of long duration in 2006–2009 led to a prolonged galactic cosmic ray (GCR) recovery to the highest level observed in the instrumental era for a variety of energetic charged particle species on Earth, over a wide range of rigidities. The remarkable GCR increase measured by several ground-based, balloon-borne, and detectors on a satellite is described and discussed. It is accompanied by a decrease in solar wind velocity and interplanetary magnetic field at 1 a.u., reaching the lowest values since measurements of the solar wind began in October 1963; the solar polar field strength (μT) measured at the Wilcox Solar Observatory (WSO) is also significantly reduced compared to prior cycles since the start of the program in 1976, the polar field in the northern hemisphere reversed in June 2012 and again in February 2014, that in the southern hemisphere reversed in July 2013. If updates of WSO data confirm the second reversal in northern solar hemisphere, it would pose a serious challenge to the Dynamo Theory. The long-term change in solar behavior may have begun in 1992, perhaps earlier. The physical underpinnings of these solar changes need to be understood and their effect on GCR modulation processes clarified. The study discusses the recent phenomena in the context of GCR modulation since 1900. These happenings affected our empirical predictions for the key parameters for the next two sunspot cycles (they may be progressively less active than sunspot cycle 24) but it enhanced support for our prediction that solar activity is descending into a Dalton-like grand minimum in the middle of the twentyfirst century, reducing the frequency of the coronal mass ejections; they determine the space weather affecting the quality of life on Earth, radiation dose for hardware and human activities in space as well as the frequency of large Forbush decreases at 1 a.u.     

A calibration neutron monitor: Statistical accuracy and environmental sensitivity

This paper is a follow-on of that of Krüger et al. [Krüger, H., Moraal, H., Bieber, J.W., Clem, J.M., Evenson, P.A., Pyle, K.R., Duldig, M.L., Humble, J.E. A calibration neutron monitor: energy response and instrumental temperature sensitivity. J. Geophys. Res. 113, A08101, doi:10.1029/2008JA013229, 2008], that describes the characteristics of a pair of calibration neutron monitors that were developed to intercalibrate the count rates of the world’s neutron monitors against each other. Such an intercalibration will allow the calculation of energy (rigidity) spectra, which will enhance the quality of the neutron monitor data. Krüger et al. (2008) investigated the energy and temperature response of the calibrators. This paper studies the statistical accuracy of the calibration procedure, its repeatability, and the sensitivity to its environment. The paper concludes with a calibration procedure that can minimise the uncertainties caused by these five effects, or at least correct for them.