"北斗"陆基增强系统岸台同步技术研究

导航信号同步技术是无线电导航系统的关键技术.本文介绍了"北斗"陆基增强系统的技术方案,对该系统导航信号同步技术进行了分析.利用"北斗"单向授时技术实现导航台时钟同步;采用CPLD器件设计同步脉冲提取电路及同步调整电路;利用直接频率合成技术产生高精度、高稳定度的扩频伪码时钟.实测数据分析表明,通过"北斗"授时可以保证陆基增强系统的导航台链具有较高的时钟同步精度.     

On the early phase of relativistic solar particle events: Are there signatures of acceleration mechanism?

Many physical processes precede and accompany the solar energetic particles (SEP) occurrence on the Earth’s orbit. Explosive energy release on the Sun gives rise to a flare and a coronal mass ejection (CME). X-ray and gamma emissions are believed to be connected with flares. Radio emission is signature of disturbances traveling through the corona and interplanetary space. Particles can gain energy both in the flare and the accompanying wave processes. The beginning of the SEP events has the advantage of being the phase most close to the time of acceleration. Influence of interplanetary transport is minimal in the case of first arriving relativistic solar protons recorded by ground based neutron monitors in so called ground-level enhancements (GLE). The early phase of the SEP events attracts attention of many scientists searching for the understanding of particle acceleration. However, they come to the opposite conclusions. While some authors find arguments for coronal mass ejections as a sole accelerator of SEPs, others prove a flare to be the SEP origin. Here, the circumstances of SEP generation for several GLEs of the 23rd solar cycle are considered. Timing of X-ray, CME, and radio emissions shows a great variety from event to event. However, the time of particle ejection from the Sun is closer to maximum of X-ray emission than to any other phenomena considered. No correlation is found between the particle fluxes and the CME characteristics.     

快变分量观测与基本分量特性

本文对太阳２２周峰年期云南天文台日冕射电频谱仪观测到的６０个快速事件作了分析。从中获得了尖峰辐射、增强噪暴、快速起伏、类尖峰、叠加脉冲五种快变型别，对它们的亮温度、叠加特性、特征时间、辐射源尺度、偏振特性以及辐射机制六个方面作了分析研究后，对射电爆发、缓变分量和宁静太阳的辐射特征参量也作了研究，从而得出基本分量特性。     

Ionospheric responses to the 21 August 2017 great American solar eclipse – A multi-instrument study

Herein, we report on the ionospheric responses to a total solar eclipse that occurred on 21 August 2017 over the US region. Ground-based GPS total electron content (TEC) data along with ground-based measurements (Millstone Hill Observatory (MHO) and digital ionosondes) and space-based measurements (COSMIC radio occultation (RO) technique) allowed us to identify eclipse-associated ionospheric responses. TEC data at ~20°, ~30°, and ~40°N latitudes from the west to east longitudes show not only considerable depression but also wave-like characteristics in TEC both in the path of totality and away from it, exclusively on the day of eclipse. Interestingly, the observed depressions are associated with lesser (higher) magnitudes at stations over which the solar obscuration percentage was meager (significant), a clear indication of bow-wave-like features. The MHO observes a 30% reduction in F₂-layer electron densities between 180 and 220 km on eclipse day. Ionosonde-scaled parameters over Boulder (40.4°N, 100°E) and Austin (30.4°N, 94.4°E) show a significant decrease in critical frequencies while an altitude elevation is seen in the virtual heights of the F-layer only during the eclipse day and that decreases are associated with wave-like signatures, which could be attributed to eclipse-generated waves. The estimated vertical electron density profile from the COSMIC RO-based technique shows a maximum depletion of 40%. Relatively intense and moderate depths of TEC depression, considerable reductions in the F₂-layer electron densities measured by the MHO and COSMIC RO-measured densities at the F₂-layer peak, and elevations in virtual heights and reduction in the critical frequencies measured by ionosondes during the eclipse day could be due to the eclipse-induced dynamical effects such as gravity waves (GWs) and their associated electro-dynamical effects (modification of ionospheric electric fields due to GWs).     

射频识别卡读写模块的设计

射频识别卡读写模块是射频卡读写器的核心.根据ISO14443协议,运用现代通信与信号处理的方法,采用最新的RISC指令单片机,设计了射频识别卡的读写模块.该模块没有使用专用的硬件ASIC和功率放大管,纯粹采用软件实现了硬件ASIC的功能.同时它性能稳定、价格低廉,对卡的读写距离在0~10cm.      

TD-SCDMA 中外环功率控制的研究

CDMA系统是干扰受限的系统,降低干扰可以提高系统的容量.TD-SCDMA系统的功率控制就是在保证用户的QoS前提下,降低发射功率,减少系统干扰从而增大系统的容量.本文介绍了TD-SCDMA中外环空率控制的算法,并且分析了功率控制参数对系统性能的影响.     

超短波电台自动检测与故障诊断系统设计

介绍了超短波电台自动检测系统与故障诊断系统的功能,并根据功能要求进行了硬件电路的设计,采取面向信号的ATLAS语言进行软件设计和建立在专家知识输入故障推理模型.该系统经使用证明,检测结果精确,检测效率较高.     

复杂环境下的A/C模式信号处理算法及其实现

本文基于软件无线电的思想,提出一种复杂环境下的A/C模式信号处理算法,该算法从脉冲识别,A/C模式框架判决以及信息代码提取三个方面进行了研究,在识别多目标混叠、拒绝目标幻影,避免异步串扰方面,达到了较好的效果,并在FPGA上实现了该算法.     

电磁散射场和雷达散射截面积的计算

计算了绕二维物体的时域电磁散射场的空间分布和雷达散射截面积 (RCS).通常的电磁场计算是频域的,采用高频计算方法,而流场计算是时域的.由于以研究流场--电磁场优化设计计算为目的,需要统一采用时域计算,因此重点采用矢通量分裂法这种时域方法计算了RCS ,通过将特征值分裂为正负两部分,抑制了各自的误差.此外,采用LaxWendroff方法作为对照.两种方法的结果一致.     

X-ray and radio observations of the galaxy cluster 3C 129

The galaxy cluster 3C 129 contains two radio galaxies, the prototypical head tail radio galaxy 3C 129 and the weaker radio galaxy 3C 129.1. The tail of the first radio galaxy extends over more than 15′ across the sky. In this paper, we report on Chandra spectroscopy observations of the galaxy cluster, complemented by new and archival radio data taken with the Very Large Array (VLA) at 0.33, 1.4, 5, and 8 GHz and by HI-observations performed with the dominion radio astrophysical observatory (DRAO). We describe the Chandra results on the properties of the Intra-Cluster Medium (ICM) and discuss extended X-ray emission detected from the host galaxy of the radio galaxy 3C 129.1 and from the inner jet of the radio galaxy 3C 129. Finally, we report on the results of an ICM/radio plasma pressure balance study along the tail of the radio galaxy 3C 129.