一种改善GPS接收机载波相位连续性的相位预测方法

针对GPS信号受短时遮挡等影响导致载波相位不连续问题，提出一种基于载波开环跟踪的相位预测方法。通过对失锁通道的多普勒进行精确预测实现对载波相位进行开环跟踪，重点改善接收机晶振钟漂对多普勒估计精度的影响。基于软件接收机对该方法进行性能评估，在部分GPS信号连续中断15 s情况下，其估计的载波相位误差小于1/4周的概率在90%以上。     

CFL-03型风廓线雷达故障分析诊断技巧

现在风廓线雷达已被广泛应用在局地天气预报、空中管制、大气污染预防等方面,对国民经济的发展具有重要的意义。随着雷达使用年限的增加,雷达设备故障率也在增加。由于CFL-03型风廓线雷达已经实现了全固态、模块化设计,许多气象局都订购了相关的备件,因此只要对设备进行故障诊断,判断出故障的位置,进行备件更换,设备就可以恢复正常工作。按照CFL-03型风廓线雷达的组成,对故障部位进行分析,结果表明,常见故障发生的地方一是监控组合的监控板,二是故障发生点为接收机的标频组件、基准组件等,三是故障发生点为发射机的功合部分、波控的波束转换板,四是故障点为天线的一分六公分器。在故障判断过程中,最简单的方法就是利用分机组合上的故障指示灯和软件界面上的故障信息指示表来判断。此外,利用三用表、示波器、频谱仪和矢量网络分析仪等可以进一步判断故障。     

Hard X-ray all-sky imaging with BATSE/CGRO

The large Area Detectors (LADs) of the BATSE experiment aboard the Compton Gamma-ray Observatory have been used recently as the first hard X-ray all-sky imager at energies between 20 keV and 300 keV. The Earth occultation process is formulated in terms of a curved Radon transform convoluted by a step transform in a selected field of view (FOV) ranging from 5°×5° to 40°×40°. The Maximum Entropy Method is then used to reconstruct an image in the hard X-ray sky. Multiple images of different regions of the sky can be produced simultaneously. A source location accuracy of 0.1° for strong sources and a sensitivity limit of 100 mCrab have been achieved in an one-day integration period.Invited Paper on Imaging in High Energy Astronomy, Sept., 1994, Capri, Italyalso Universities Space Research Association     

CINRAD/CD接收机疑难故障案例诊断分析

针对CINRAD/CD无机内测试信号的疑难故障案例,介绍如何借助大型电子设备规范化维修的理念和方法,结合雷达系统原理和信号流程,综合运用原理分析法、越级法、测量法、代替法等故障诊断方法进行分析与判断,逐步缩小故障排查范围,从而达到快速定位及排除故障的目的。最终确定该故障是由于接收与监控分机间的信号线断开,造成控制码没有送至微波组件内单刀双掷微波开关所导致的。文中提供了该类型故障的规范化维修流程,其诊断方法和思路可广泛应用于CINRAD技术保障工作中。     

一种BDS/GPS接收机单频定位精度分析

针对基于多模导航卫星系统单频接收机在非完好性条件下的数据缺失问题,该文提出了一种能有效提高多模单频接收机定位精度的方法。通过对观测数据非完好性的明确界定、典型情况分析和单频定位方法研究,实现了非完好条件下多模单频数据的有效解算。通过研究证明:在一定的非完好条件下,BDS/GPS单频接收机数据经过该方法的数据处理能够得到较好的定位精度。     

GPS系统下RAIM算法可用性及结果分析

介绍了接收机自主完整性监测(RAIM)算法的故障检测及其可用性原理,结合航空用户对完好性需求,通过仿真计算,得到了GPS系统下不同截止高度角条件下、不同飞行阶段的RAIM算法的可用性结果,并且给出了中国区域内5°×5°格网点的RAIM最大和平均中断时间,分析了截止高度角、可视卫星个数和DOP值等因素对RAIM算法可用性的影响。     

Investigation of LO-Coupled Noise for a Sideband Separation Superconducting SIS Receiver

The Superconducting Superconductor-Insulator-Superconductor (SIS) receivers have become the preferred method for (sub)millimeter-wave radio astronomical observations due to the extremely low receiver noise temperature. The coupling noise of the local oscillator (LO) system is also a part of the receiver noise. In many years of astronomical observations, it is found that the LO-coupled noise cannot be completely ignored, which has a certain impact on the sensitivity of astronomical observations. The noise temperature of the superconducting SIS receiver was tested using two different kinds of signal generators as the primary signal source of the LO system. It is found that the base noise output by the signal generator can be coupled into the receiver to increase the receiver noise. By adding a narrow band filter to the output of the signal generator, the base noise of the signal generator can be filtered out, and this part noise of the receiver can be eliminated, the overall noise of the receiver is reduced, and the sensitivity of the telescope is improved.     

卫星导航接收机中锁频环的两种实现方式

对卫星导航接收机中的锁频环进行了研究，主要涉及锁频环的鉴别器算法、环路调节的两种方式，并对这两种实现方式作了仿真。     

C波段卫星信号接收机低噪声放大器的设计

介绍了一个应用于C波段卫星信号接收机的低噪声放大器(LNA)的设计过程。为达到低噪声和高增益的目标,该低噪声放大器是利用低噪声的PHEMT晶体管ATF36077(用在第一级)和噪声性能良好的微波单片放大器MGA86576(用在第二级)级联设计完成的。测试结果表明,该低噪声放大器的性能达到了预定指标:在3.8 GH至4.2 GHz工作带宽内噪声系数NF≤0.7 dB,增益≥36 dB,1 dB带宽约350 MHz。