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。     

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。     

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.     

Mean energy of response to galactic cosmic ray spectrum: IMP 8 and Climax neutron monitor

Solar modulations of galactic cosmic ray (GCR) intensity contain a wealth of information about their transport in the heliosphere. To extract this information from the data one studies the dependence of the observed modulations on the mean energy of response of detectors providing data for the analyses. There is a great deal of confusion about the detector energy response to GCR spectrum in the literature. We present a preliminary report on the computations of the mean energy of response for the Climax neutron monitor (CL/NM) and IMP 8 cosmic ray nuclear composition instrument to GCR protons for 1973–1998, covering the solar cycles 21 and 22. We find that for penetrating proton channel on IMP 8 the mean energy changes by a factor of over two whereas for the neutron monitor the change is only 21%. However, the corresponding change for the computed modulation function is a factor of about 3.5.     

多载波调制结合Turbo编码技术的性能分析

多载波调制是一种有效克服衰落信道频率选择性的技术,从而显著减少码间干扰(ISI)。Turbo码以其接近香农极限的工作性能受到人们的注目,它能在极低信噪比条件下提供可靠通信。把多载波调制与Turbo 编码结合起来能够对整个系统提供显著的性能增益。本文试图对采用这两种技术的通信系统给出性能上的评估。     

气动FA补偿变结构Bang-Bang位置伺服算法

 首先提出了一种基于两位两通高速开关阀的无杆气缸脉宽调制（PWM）控制方案,为气缸提供了中位截止机能。然后针对Bang-Bang控制算法中存在的超调和振荡现象,提出了摩擦力和加速度（FA）补偿的变结构Bang-Bang算法。该算法综合位置和速度误差的影响构造了加速度方向切换评价函数,考虑了摩擦力对控制量设定的影响,分别依据阶跃函数、线性函数和反正切函数对活塞加速度值进行动态设定,实现了运动过程中对活塞摩擦力的补偿和加速度的调整。最后,利用该算法进行了无杆气缸的带载伺服定位试验,对3种加速度设定函数的控制效果做了比较。结果证明FA补偿变结构算法在提高气缸定位精度方面有显著效果。     

双轴连续旋转调制捷联惯导系统大失准角初始对准技术

由于可以补偿惯性器件在三个轴向上的输出误差,双轴旋转调制技术被广泛应用于捷联惯导系统(SINS)。选择了一种合理且实用的十六次序双轴转位方案,并对其调制原理和误差进行了分析。初始对准技术是捷联惯导系统的一项重要技术,其对准精度直接决定了后续导航的精度。在粗对准完成后,当姿态误差角较大时,后续的精对准误差模型呈非线性特性,故选择了滤波精度高、稳定性强的平方根容积Kalman滤波算法(SCKF)来解决这一问题。考虑到在实际对准过程中,量测噪声的统计特性易发生变化,将SCKF算法与Sage-Husa算法相结合,在传统Sage-Husa SCKF算法的基础上提出了一种改进的自适应滤波算法(ASCKF)。该算法采用QR分解来完成对噪声协方差的平方根矩阵估计,从而避免了传统Sage-Husa SCKF算法中所估噪声协方差矩阵不正定的问题。最后,通过仿真证实了ASCKF算法可被很好地应用于量测噪声统计特性发生变化的初始对准中。