Operational modal parameter identification with colored noise excitation

Operational Modal Analysis (OMA) refers to the modal analysis of a structure in its operating state. The advantage of OMA is that only the output vibration signal of a system is used in the analysis process. Classic OMA is based on the white noise excitation assumption and many identification methods have been developed in both time domain and frequency domain. But in reality, many environmental excitations are not compliance with the white noise assumption. In this paper, a method of half power bandwidth analysis is applied to power spectrum analysis to deal with the colored noise and trapezoidal spectral excitation. The modal frequencies and modal damping ratios are derived and the error caused by trapezoidal spectral and colored noise excitation are analyzed. It is proved that the OMA algorithm based on the white noise assumption can be extended to the colored noise environments under certain conditions. Finally, a simulation example with a cantilever beam and a vibration test with four kinds of colored noise and trapezoidal spectrum base excitation are carried out and the results support the proposed method.     

多媒体流处理器中缓冲器的体系结构设计

传统微处理器体系结构不能很好地匹配媒体处理应用的特点.针对处理器与存储器之间日益增长的性能间隙问题,分析了传统微处理器对媒体处理应用的通讯瓶颈;通过分析Cache存储器的特点,得出了传统的Cache结构并不适合现代媒体处理应用的结论,讨论了目前针对处理器通讯瓶颈的一些解决办法;提出了一种以大容量流寄存器堆替代Cache作为中间缓冲器,并能适合于媒体处理应用的金字塔存储层次体系结构设计.该体系结构具有三级并行数据带宽存储层次,即片外SDRAM、全局寄存器堆和局部寄存器堆.三级并行存储层次所能提供的带宽依次提高一个数量级,带宽之比为1∶16∶256,从而可以有效地支持卫星遥感图像预处理对数据带宽的需求.      

通信系统电磁兼容性设计

一个设计不好的无线电发射机, 工作时产生的谐波十分严重, 而接收设备又对电磁干扰非常敏感。本文介绍了发射机谐波的抑制方法和接收机抗干扰技术体制, 实现自适应通信, 确保通信质量。     

低频噪声源的测试方法

介绍了针对低频噪声源三种参数的测试方法.讨论了低频噪声源的最大输出功率、噪声输出幅度以及噪声带宽测试的实现途径.     

基于广播内存网络的无人机传感器仿真系统

讨论了一种基于广播内存网络的无人机飞行传感器仿真系统的设计与实现。系统硬件平台采用了基于网络的多机分布式体系结构。系统软件采用了VC＋＋6.0设计语言。该系统能够模拟无人机各种真实机载传感器信号及完成其它I／O信号处理，具有高实时性、高可靠性的特点。     

高性能嵌入式信号处理应用中的互连结构

目前,由多个处理器构成的高性能嵌入式信号处理系统中,处理器之间、信号处理模块之间的通信带宽已经成为整个应用系统性能的瓶颈,如果没有与高性能处理器同步的互连结构方案,就无法调动多个处理器的全部处理潜能。本文对高性能嵌入式信号处理应用中用到的几种互连结构及实现方式进行比较、分析,并且讨论互连结构的发展趋势。     

突发通信信号的降维检测方法及带宽参数分析

在突发通信信号检测中,在频率、带宽进行二维搜索的检测方法计算量大,提出了可减少计算量的降维检测方法,该方法在单一检测带宽下进行频率搜索检测突发通信信号。对其带宽参数选择进行了分析。理论计算和仿真表明,降维检测器用于单一速率信号检测时,当检测带宽与信号带宽一致时具有与二维检测器相同的检测性能,当检测带宽与信号带宽相差一倍时,信噪比损失2dB左右;用于混合速率突发信号检测时,最佳带宽与速率的概率分布、信噪比等多种因素有关;对发送功率不变的各速率均匀分布的混合速率突发信号,检测带宽匹配于最大信号带宽可在较高信噪比时获得最高的平均检测概率。这些分析为降维检测器的带宽参数选择提供了依据。     

LTPB网络带宽分配策略的实时性能研究

研究LTPB(线性令牌传递总线)在通信网络中保证消息实时传输的带宽分配问题.LTPB网络带宽的分配是以保证网络消息的实时传输为目标的,网络中关键参数(一定时间内发送消息的最小量)的准确与否将关系到网络带宽分配的合理性和有效性.通过对带宽分配方法实时特性的分析,发现了当前分析方法中的不足,提出了"最差情形"的概念,并以此建立了合理的推导模型,得出了有关LTPB网络实时性分析的关键性结果,并为下一步寻求更优的带宽分配方法提供了可靠的分析基础.      

基于效用最大化的DVB-RCS跨层动态带宽分配

针对已有效用函数的动态带宽分配(DBA)模型未考虑物理层信道条件来完成DVB-RCS(Digital Video Broadcasting-Return Channel via Satellite)卫星通信网的DBA,从而导致吞吐量下降这一缺点,本文提出一种跨层效用函数DBA模型.该模型建立基于信道条件的效用函数,以实现效用最大化的DBA,因此转化为非线性整数规划问题的求解.同时提出一种基于等效用增量的Greedy迭代算法求解该问题,求出效用最大化的带宽分配向量,降低了传统Greedy算法的计算量.仿真结果表明该模型在保证回传信道卫星终端(Return Channel Satellite Terminal,RCST)用户公平性的同时,提升DVB-RCS卫星通信网的吞吐量.     

Black hole accretion and X-ray spectra of QSOS

Changes in Eddington accretion ratios are thought to result in X-ray spectral index changes in Galactic binary black hole systems. Objects with higher Eddington ratios have softer X-ray spectra. Can we apply this result to much more massive black hole systems such as QSOs? If so, X-ray observations will give us valuable insight into the physics of QSOs. Among QSOs, X-ray spectral index is part of a large set of correlated optical and UV observational properties, especially optical Fe II and [O III] strengths in the Hβ region. To investigate whether this set of correlations is related to Eddington ratio, we use as probes, BALQSOs that have been suggested to be youthful super-accretors. We conducted infrared spectroscopy of the Hβ rest wavelength region for a sample of BALQSOs and compared line measurements with those for high and low redshift non-BAL QSOs. Hβ line widths and bolometric luminosity are used to calculate QSO black hole masses and Eddington ratios. Our results support the hypothesis that optical Fe II and [O III] line strengths are Eddington ratio indicators in QSO central engines. A possible explanation is that strong Fe II and weak [O III] indicate abundant cold gas that could fuel near Eddington accretion.