基于生物学同步模型的WSN群同步算法研究

在研究现有无线传感器网络时间同步算法的基础上,为进一步满足大规模网络对同步算法精度和扩展性的需求,将生物学同步模型引入无线传感器网络中,提出一种分布式的群时间同步算法,并进行仿真验证。结果表明,该算法能够使具有不同初始相位的网络节点最终达到相位同步,满足网络同步要求。     

基于网络的GNSS共视时间比对数据传输系统的设计与实现

为了实现远程时间同步中的共视数据自动、连续传输,提出了基于TCP/IP协议来实现C/S模式的数据传输方案。阐述了数据发送端与接收端的传输原理和实现方案。发送端通过串口采集数据并通过网络将其传输到接收端,接收端接收发送端的数据并对其检验并保存。设计了发送端与接收端自动重连接功能,实现了数据传输的连续性。测试表明:采用基于TCP/IP协议和C/S模式的数据传输系统能够实现共视数据自动、连续、可靠的传输。     

基于GNSS CV的精密时间服务系统的设计与实现

通过研究GNSS(global navigation satellite syetem,全球导航卫星系统)共视远程时间传递技术,并结合现代网络通信技术,搭建了基于GNSS CV(common-view,共视)的精密时间服务系统的硬件平台。利用中国科学院国家授时中心保持的精确时间UTC(NTSC)和GNSS共视接收机观测数据,实现了用户与国家授时中心之间的在线数据传输和比对处理,为用户时间与UTC(NTSC)之间的高精度时间同步提供了一种解决方案。     

First XMM-Newton observations of strongly magnetic cataclysmic variables – I. Spectral studies of DP Leo and WW Hor

We present an analysis of the X-ray spectra of two strongly magnetic cataclysmic variables, DP Leo and WW Hor, made using XMM-Newton . Both systems were in intermediate levels of accretion. Hard optically thin X-ray emission from the shocked accreting gas was detected from both systems, while a soft blackbody X-ray component from the heated surface was detected only in DP Leo. We suggest that the lack of a soft X-ray component in WW Hor is owing to the fact that the accretion area is larger than in previous observations with a resulting lower temperature for the re-processed hard X-rays. Using a multi-temperature model of the post-shock flow, we estimate that the white dwarf in both systems has a mass greater than 1 M_⊙. The implications of this result are discussed. We demonstrate that the 'soft X-ray excess' observed in many magnetic cataclysmic variables can be partially attributed to using an inappropriate model for the hard X-ray emission.     

First XMM-Newton observations of strongly magnetic cataclysmic variables – II. Timing studies of DP Leo and WW Hor

XMM-Newton was used to observe two eclipsing, magnetic cataclysmic variables, DP Leo and WW Hor, continuously for three orbital cycles each. Both systems were in an intermediate state of accretion. For WW Hor we also obtained optical light curves with the XMM-Newton Optical Monitor and from ground-based observations. Our analysis of the X-ray and optical light curves allows us to constrain physical and geometrical parameters of the accretion regions and derive orbital parameters and eclipse ephemerides of the systems. For WW Hor we directly measure horizontal and vertical temperature variations in the accretion column. From comparisons with previous observations we find that changes in the accretion spot longitude are correlated with the accretion rate. For DP Leo the shape of the hard X-ray light curve is not as expected for optically thin emission, showing the importance of optical depth effects in the post-shock region. We find that the spin period of the white dwarf is slightly shorter than the orbital period and that the orbital period is decreasing faster than expected for energy loss by gravitational radiation alone.     

一种基于GNSS的可驯频标的设计与实现

重点介绍了GNSS可驯频标软件设计方法。在软件设计中,采用了滑动中位数方法以滤除测量数据中的奇异值;利用了Kalman滤波器对测量时差数据进行滤波以抑制测量噪声;提出了一种改进型的压控电压产生方法。采用GPS定时接收机1 PPS信号作为参考基准,对原来准确度为1×10-9恒温晶振进行驯服,驯服后频率准确度优于2×10-11。     

基于Wi-Fi的NTP无线授时服务器的设计与实现

为满足需求,给出了一种基于Wi-Fi的NTP无线授时服务器的设计方案。该服务器用GPS作为时间源,将GPS接收机输出的时间信息传送给ARM控制器,进行时码信息的采集与处理,通过Wi-Fi无线收发模块将服务器连接到网络层,并采用NTP协议实现授时。授时精度在局域网内可达到1 ms。     

基于W500的NTP时间服务器设计

针对局域网领域对时间同步的要求,主要利用微控制器STM32和单片网络接口芯片W5100为核心搭建硬件平台来设计一个高精度、高吞吐量的NTP时间服务器系统,为客户端提供高精度的时间信息,从而实现客户端与服务器时间同步的功能。实验及分析表明,该系统运行稳定,能够实现网络时间同步。     

基于FPGA的IRIG-B（DC）码的解码方案的设计与实现

IRIG-B码是国际上通用的时间码格式,广泛应用于各种系统的时间同步。针对IRIG-B（DC）码的调制特性,介绍一种基于FPGA的B码解调方案。重点描述了如何在同步时序中准确提取秒同步信号并解调B码中包含的时间信息。整个方案中采用Verilog HDL语言进行设计,已成功实现,并给出了验证结果。     

基于DDS技术的Loran—C信号源的杂散信号抑制的分析与实现

采用直接数字频率合成（DDS）技术设计的Loran—C信号源,具有输出杂散多且难以预测的缺点。基于对DDS基本原理的研究分析,针对DDS输出信号存在的相位舍位杂散问题,对其关键部位的相位累加模块进行优化设计,并基于FPGA技术,在QuartusII环境下完成了对Loran．C信号源的实现与仿真验证。结果表明,通过优化的设计算法能够产生失真小,稳定度好的输出波形,从而验证了该方法抑制杂散的有效性与可行性。     

The design and implementation of a ROACH2+GPU based correlator on the Tianlai dish array

A digital correlator is a crucial element in a modern radio telescope. In this paper, we describe a scalable design for the correlator system of the Tianlai pathfinder array, which is an experiment dedicated to testing key technologies for conducting a 21 cm intensity mapping survey. The correlator implements the FX design, which firstly performs a fast Fourier transform(FFT) including polyphase filter bank(PFB) computation using a Collaboration for Astronomy Signal Processing and Electronics Research(CASPER) Reconfigurable Open Architecture Computing Hardware-2(ROACH2) board, then computes cross-correlations by employing Graphics Processing Units(GPUs). The design has been tested both in laboratory and in actual observation.