PLL两点调制在GMSK调制器中的应用

分析了HDL数据链发信机设计中的几种GMSK调制方法;阐述了用PLL两点调制的必要性,进而给出了基于PLL的GMSK两点调制的模型。同时,对非线性模型进行线性化等效,列出它们的闭环传递函数,并通过Matlab仿真波形来观察频率响应曲线;最后对调制系统进行ADS仿真,分析系统的收敛性,通过时域、频域调制波形分析,得到最优系统参数。     

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。     

BOC调制信号的特性分析

二进制偏移载波(BOC)调制是GPS现代化后采用的新军用信号(即M码信号)的调制方式, 其设计灵活性和可变性在导航战中是非常重要的.推导并分析了不同形式BOC信号的自相关函数、功率谱、循环谱和循环谱包络切面特性,分析结果对下一步BOC信号的参数估计和模式识别具有参考价值.     

双轴旋转式激光捷联惯导系统的转位方案研究

惯性导航系统的误差随时间累积,旋转调制技术可以有效地提高惯导系统的长航时精度,旋转调制方案是决定旋转式捷联惯导系统导航精度的一个重要因素.针对双轴旋转惯导系统,相较于16次序转位方案,提出了一种新的32次序双轴旋转调制方案.根据捷联惯导系统的误差方程,推导出旋转捷联惯导的误差方程,分析了误差补偿的机理,研究了惯性器件常值偏置误差、标度因数误差和安装角误差的传播特性.仿真结果表明,32次序双轴旋转调制方案相对于16次序转位方案有明显的优势,可以有效地降低姿态角误差和经纬度误差.     

差分技术在双星快速定位通信系统中的应用

卫星定位通信系统是具有10米以内高精度的第二代卫星导航定位系统。达到高精度的关键是应用了伪随机码扩谱及差分定位技术。诸如星历误差、电离层时延变化和地球模型不准等误差,通过应用差分技术可以大部分消除。本文阐述了差分技术的应用和系统精度分析。     

Is the North Atlantic Oscillation modulated by solar and lunar cycles? Some evidences from Hurst autocorrelation analysis

Several studies have suggested that the Sun and Moon cycles affect the Earth climatic dynamics. Nevertheless, there is a long-standing controversy whether solar variability and tides can significantly generate climate change, and how this may occur. Spectral analysis of climatic indices has provided only indirect evidences of the effects of solar–tidal periodicities in the Earth climate. This work addresses the issue by considering the dynamics of the daily North Atlantic Oscillation index over the period from 1950 to 2009. In contrast to previous studies, this work proposes that external cycles can be detected in the autocorrelation dynamics rather than in the raw North Atlantic Oscillation index series. Here, the R/S-scaling analysis is used to quantify, via the so-called Hurst exponent, the presence of autocorrelations along the studied years. Fourier analysis scan of the autocorrelation series thus show two prominent spectral components near (±3%) the lunar tidal 4.425 and the solar 11 years cycles. Intermediate spectral components near 6.4, 7.75 and 8.9 years are proposed to be, at least partially, a result of energy capture from internal mechanisms into cycles resulting from the nonlinear resonance of the fundamental solar–tidal cycles. The dominant effect of the solar variability is clarified by showing that in about 70% of the studied period the sunspot number and the Hurst exponent phases are synchronized, indicating that a higher solar activity enhances the North Atlantic Oscillation index predictability.     

聚束式SAR中卷积反投影算法的快速实现

对应用于聚束式合成孔径雷达 (SAR) 成像中的卷积反投影 (CBP) 算法进行了详细研究,提出了一种基于傅里叶变换的快速实现方法,使得CBP算法的计算量得到明显降低.在传统的CBP算法中,反投影过程中的重采样通过插值实现,因而所需的插值数量巨大,导致运算效率低下.研究了图像像素之间隐含的相对位置关系之后,本文采用一系列快速傅里叶变换 (FFT)来实现反投影过程中的重采样,避免了运算量巨大的插值过程,故提高了运算效率.仿真结果证明了新算法的可行性和有效性.相比于传统的CBP算法,新算法可以提高大约85%的运算效率.由于FFT适用于并行处理,新方法在实时处理SAR系统中有一定的应用价值.     

Radial and latitudinal gradients of galactic cosmic rays in the heliosphere at solar maximum

Our understanding of galactic cosmic ray (GCR) modulation has advanced greatly in the last three decades. However, we still need an appropriate knowledge of the GCR intensity gradient. Numerical simulations of the transport particle equation allow interpretation of cosmic ray intensities in the heliosphere. We use the numerical solution of the GCR transport equation during solar maximum epoch to compute the radial and latitudinal gradients. Our analysis indicates that adiabatic energy loss plays an important role in the radial distribution of GCR in the inner heliosphere, while in the outer region the diffusion and convection are the relevant processes. The latitudinal gradient is small.     

New field of application of the IRI modeling – Determination of ionosphere transfer characteristic for radio astronomical signals

We suggest a new field of application of IRI modeling – determination of ionosphere transfer characteristic (ITC) for radio astronomical signals (RAS). VHF and HF RAS are widely used for observations of the Sun and pulsars. It is necessary to take into account possible distortions of RAS in the Earth ionosphere. However, in contrast to modern navigation systems (GPS, GLONASS, GALILEO), where very accurate reconstruction of ionosphere parameters is a built-in function, in present-day radio astronomy a retrieve of ITC has not been appropriately worked out yet. It collides with increasing requirements to accuracy of the analysis of RAS amplitude profile and to the angular and polarizing resolution of radio telescopes of new generation. We have developed a method and software for calculation of the ionosphere measure of rotation (RM) and the measure of dispersion (DM). We used the ionosphere model IRI-2001, magnetic-field model IGRF-10 and values of ionosphere total electron content as deduced from GPS measurements. The obtained values of the ionosphere DM and RM were recalculated into characteristics of phase delay, Faraday amplitude modulation and polarization changes. We made calculations for different levels of geomagnetic activity and for different angular position of radio sources as well.     

频率计数器在航天器信号频率测量中的适用性分析

从频率计数器的工作原理出发,分析了航天器测控通信中常用的调相信号、调频信号和相移键控信号的频率测量误差,给出了调相信号和调频信号的测量误差表达式。使用频率计数器对上述3种航天器信号进行了频率测量试验。理论分析和试验结果表明,频率计数器适用于航天器调相信号和调频信号的频率测量,不适用于相移键控信号的频率测量。在实际使用中,为保证测量精度,应根据被测信号的调制方式选择适当的测量方法。