中国全球卫星导航信号基本框架设计

中国的全球卫星导航信号设计必须遵循许多约束条件,具备国际可协调性,导航信号的服务类型、载波中心频率、调制方式和伪随机码序列均需参加与GPS、Galileo进行的频率协调。依据参加与GPS频率协调的参考假设文件,描述了中国的全球卫星导航信号结构、基本参数、公开导航信号的伪随机扩频码序列和二次编码序列,计算表明伪随机扩频序列的性能与GPS信号伪随机扩频序列性能相当。     

PMSM 空间矢量控制系统与MATLAB仿真

阐述了永磁同步电机(PMSM)空间矢量PWM 控制系统的原理,分析了永磁同步电机空间矢量控制方式的优劣势。综述了电机相电流坐标变换矩阵的仿真模块实现方法,展示了电机磁场PARK 变换和PARK 逆变换等从数学方程到仿真语言的转换过程,用MATLAB对该系统的电流环和速度环进行了仿真。仿真结果显示,当速度环的仿真输入为210rad/s时,速度输出的过渡过程时间达到了0.017s,超调量为4%,动态性能良好,仿真效果较为理想。     

远距离无源射频识别系统设计

文中给出射频识别系统的设计方案 ,系统采用反向散射调制技术完成从电子标签到读写器的数据传输。接收机采用零中频直接变频方案 ,电路简化 ,可有效地降低成本。抗冲突协议采用两种模式。测试结果表明 ,该方案达到了设计指标 ,可满足实际射频识别应用系统的要求     

高码率通用数字化调制技术研究

采用软件无线电技术实现遥测发射机的高码率数字化调制,构建一个开放、标准、通用的硬件平台,FM体制最高调制码速率可达20Mb/s。设计中还采用脉冲成形技术对调制信号进行预调处理,极大地提高了系统的频带利用率和射频功率的发射效率。     

CCD亚像元成像质量的调制传递函数分析

从调制传递函数MTF的定义出发,对CCD离散抽样过程的MTF进行分析,指出CCD器件的MTF不仅与输入信号的频率有关,而且与相位有关,得出了CCD器件的平均调制传递函数的计算公式。通过计算对CCD的一般成像、亚像元成像和互有四分之一像元位移的成像系统的调制传递函数进行分析比较,结果表明,理论上亚像元成像获得图像的分辨率能达到一般成像的两倍,互有四分之一像元位移的成像系统获得的图像分辨率能达到一般成像的3.74倍。在空间频率低于CCD的Nyquist频率时,多CCD的成像质量也明显好于一般成像质量。     

SARGMTI高逼真匀速运动假目标调制干扰方法

 将匀速运动目标成像特性用于干扰的目的,提出了SARGMTI高逼真匀速运动假目标调制干扰方法,确定了关键干扰参数,分析了侦察误差对干扰效果的影响,并采用三孔径干涉对消方法研究了其对GMTI的对抗性能。实验分析结果表明文中所提干扰方法可对SARGMTI形成高逼真匀速运动假目标的干扰效果,且干扰功率利用率高、对侦察依赖性较低,是一种先进有效的干扰方法。     

一种应用于低频电磁波通信的快响应原子磁强计

相较于传统线圈,原子磁强计作为低频电磁波通信信号磁传感接收器具有体积小、灵敏度高的优势。基于射频-光双共振原理实现原子的宏观极化和相干进动,并通过探测磁矩横向分量来获得待测磁场信息,最终实现一台灵敏度500 fT/Hz^1/2@1～5 Hz,响应带宽3.5 kHz的原子磁强计。并利用该原子磁强计作为磁传感器对频率200 Hz、磁场分量幅度10 nT的电磁波开展了通过探测磁场分量接收通信信号的实验,实现码率200/s的电磁波通信信号的接收,验证了该磁强计作为接收机接收低频电磁波通信信号的能力。     

高速TCM传输技术及其应用

首先讨论了传统数字传输体制的特点，找出传统调制与编码的分离独立设计是制约数字通信系统性能进一步提高的本质根源；并由此论述了编码与调制相结合的高速数字传输体制，重点讨论了网格编码调制(TCM)技术的基本特点、集合分割映射原理、性能估算，并对TCM在AWGN信道中的性能进行了仿真。     

Transient Effects and Disturbed Conditions

In the present phase of the solar cycle no big transients leading to strong modulation had been observed after 1991. Apart from a few minor disturbances cosmic rays were still recovering to a new intensity maximum. It was suggested, therefore, that existing literature from previous cycles should be critically reviewed. The scene was set by the introductory papers on— phenomenology of cosmic ray modulation in successive solar cycles throughout the heliosphere— the present state of models for long term modulation and their shortcomings— the relation between cosmic ray variations and the magnitude of the interplanetary magnetic field (the CR-B-relation)— charge dependent effects.In the discussions, the study of propagating diffusive disturbances and the CR-B-relation played a central role. The difference was stressed between isolated transient disturbances in the inner solar system (Forbush decreases), and the long lasting, step-like decreases caused by merged interaction regions in the outer heliosphere. The recovery rates following the step-like decreases vary with the phase in the 22-year solar cycle. In some cases this requires a modification of existing drift models. In the outer heliosphere, the CR-B-relation leads to the result 1/ between the diffusion coefficient and the field magnitude . This simple result is a challenge for theoreticians to derive the perpendicular diffusion coefficient fromfirst principles. The three articles in this report essentially follow the list of open points and arguments just presented.The article "Observations and Simple Models" is organised around the model of a propagating diffusive barrier, its application to Forbush effects in the inner heliosphere and to decreases caused by merged interaction regions in the outer heliosphere. Acomparison of observed Forbush decreases with model predictions requires a careful separation of the two steps related to the turbulent region behind the shock front and the closed magnetic field regions of the ejecta (the interplanetary counterparts of coronal mass ejections). It is shown that models for propagating disturbances can be used to derive values of the diffusion coefficients phenomenologically, not only during the disturbance, but also in the ambient medium.The "Modeling of Merged Interaction Regions" summarizes the dynamic and time-dependent process of cosmic ray modulation in the heliosphere. Numerical models with only a time-dependent neutral sheet prove to be successful when moderate to low solar activity occurs but fail to describe large and discrete steps in modulated cosmic rays when solar activity is high. To explain this feature of heliospheric modulation, the concept of global merged interaction regions is required. The com-bination of gradient, curvature and neutral sheet drifts with these global merged interaction regions has so far been the most successful approach in explaining the 11-year and 22-year cycles in the long-term modulation of cosmic rays.The "Remarks on the Diffusion Tensor in the Heliosphere" describe available theories of perpen-dicular diffusion and drift, and discuss their relevance to cosmic rays in the heliosphere. In addition, the information about diffusion coefficients and spatial gradients obtained from the analysis of steady state anisotropies at neutron monitor energies is summarized. These topics are intimately related to the other two articles. They are also part of the general discussion about the "Diffusion Tensor throughout the Heliosphere" which played an important role in all working groups.     

Extended dynamic system modulation for real-time obstacle avoidance

In this paper, a novel real-time obstacle avoidance method based on Dynamic System(DS), is proposed. The proposed method ensures the impenetrability of multiple convex obstacles by online modulating the original velocity field of the DS. It can be applied to perform obstacle avoidance in the state space of the DS with both autonomous and non-autonomous DS-based controllers. While realizing the obstacle avoidance, the equilibrium points of the original DS can be saved. The modulation matrix form ...