测量时刻偏差对单星定轨误差的影响分析

为评估测量时刻偏差对单星定轨等效测量误差的影响,根据单星定轨处理策略分析了其理论模型,指出测站接收机的测量时刻偏差由测站时钟钟差以及测量时刻不准确度等组成。试验数据分析表明,测站钟差经一阶多项式拟合后的残差可近似为零均值的测量噪声;数值仿真结果表明,卫星信号发射时刻1ms误差导致GEO、IGSO、MEO三种卫星的等效测距误差分别为006cm、40cm、80cm。     

合理运用SI技术快速收敛高速数字电路设计

随着数字电路集成度和工作频率的不断提高,信号完整性(Signal Integrity, SI)问题在产品研制过程中越来越突出。以惯导系统中的某导航计算机为例,针对故障信号回路,使用仿真软件对其SDRAM时钟信号进行信号完整性仿真,并进行优化设计。通过对比优化前和优化后的仿真与测量结果,验证了由于端接参数不匹配造成SDRAM时钟信号的非单调性畸变问题。仿真与测量结果表明,在产品研制流程中加入信号完整性仿真环节有利于设计快速收敛,提前规避风险,缩短研发周期,降低设计成本,提高电路产品的可靠性和电磁兼容性。     

Highlights about the performances of storm-time TEC modelling techniques for low/equatorial and mid-latitude locations

A statistical evaluation of storm-time total electron content (TEC) modelling techniques over various latitudes of the African sector and surrounding areas is presented. The source of observational TEC data used in this study is the Global Navigation Satellite Systems (GNSS), specifically the Global Positioning Systems (GPS) receiver networks. For each selected receiver station, three different storm-time models based on empirical orthogonal functions (EOF) analysis, non-linear regression analysis (NLRA) and Artificial neural networks (ANN), were implemented. Storm-time GPS TEC data used for both development and validation of the models was selected based on the storm criterion of $\mathit{Dst}?-50$ nT or $K_p?4$ to take into account both coronal mass ejections (CMEs) and co-rotating interaction regions (CIRs) driven storms, respectively. To make an independent test of the models, storm periods considered for validation were excluded from datasets used during the implementation of the models and results are compared with observations, monthly median values, and International Reference Ionosphere (IRI-2016) predictions. Considering GPS TEC as reference, a statistical analysis performed over six storm periods reserved for validation revealed that ANN model is about 10%, 26%, and 58% more accurate than EOF, NLRA, and IRI models, respectively. It was further found that, EOF model performs 15%, and 44% better than NLRA, and IRI models, respectively, while NLRA is 25% better than IRI. On the other hand, results are also discussed referring to the background ionosphere represented by monthly median TEC (MM TEC) and statistics are provided. Moreover, strengths and weaknesses of each model are highlighted.     

路网匹配定位方法研究

针对车载惯性导航设备由于其惯性器件随时间漂移产生误差导致系统定位精度逐渐变差的问题,提出了一种路网匹配定位方法以提高车载导航系统的综合定位精度,该方法基于视觉测量原理通过双目摄像装置采集道路周边环境特征进行匹配定位,介绍了匹配定位的基本原理和系统实现所需的关键技术,通过实际跑车测试,验证了该方法的合理性和可行性。     

不同强度磁暴期间热层大气密度响应特征分析

利用CHAMP卫星数据,对2002-2008年12个不同强度磁暴事件期间的热层大气密度变化特征进行分析,并研究对应磁暴期间大气模式NRLMSISE-00分布特征.结果表明,大磁暴期间日侧大气密度峰值从高纬到低纬的时间延迟为2h,中小磁暴期间的延迟时间为3～4h;春秋季暴时大气密度分布基本呈南北对称分布,而夏冬季大气密度的分布是夏半球大于冬半球,春秋季暴时大气密度大于夏冬季;NRLMSISE-00大气模式得到的热层大气密度很好的体现了半球分布以及季节分布的特征,但模式模拟结果偏小;Dst指数峰值比ap指数峰值更能反应大气密度的变化情况.      

RNSS/INS深耦合高动态导航接收机测试方法研究CSCD

卫星导航和惯性导航采用深耦合方式实现导航作为世界上最先进的导航形式,在国防中的应用越来越广泛,但其在高动态下的性能需要验证。当前针对深耦合高动态下导航接收机的测试研究较少,本文介绍了基于卫星信号模拟器的测试系统组成及测试用高动态场景,运用模拟测试原理,通过对导航接收机在高动态下定位速度和跟踪灵敏度的测试及其结果分析,验证了导航接收机的深耦合功能,对此类接收机的测试方法进行了初步探究。     

基于导航姿态解算的光纤陀螺平台低频角振动测试方法研究CSCD

为准确评价光纤陀螺平台的低频角振动特性,提出了一种基于导航姿态解算的光纤陀螺平台低频角振动测试方法。首先,通过角振动台精确模拟载体的低频角振动状态,并通过光纤陀螺平台飞行导航过程中的断调平差分信号,实现平台框架角度信号与角振动台激励角度信号的数据同步;然后,利用平台式惯导系统的导航姿态解算方法,实时解算低频角振动过程中光纤陀螺平台的台体姿态,并通过坐标系转换得到平台基座系相对于地理系的实时姿态;最后,通过对光纤陀螺平台稳定回路的幅相特性分析,得到低频角振动激励下稳定回路的幅值和相位特性,实现对光纤陀螺平台角动态特性的准确评估。     

Study of maximum electron density NmF2 at Karachi and Islamabad during solar minimum (1996) and solar maximum (2000) and its comparison with IRI

The monthly hourly medians of maximum electron density, N_mF₂, at two Pakistani ionospheric stations, Karachi and Islamabad, have been determined for solar minimum (1996) and solar maximum (2000) and compared with IRI predictions using the URSI coefficients. At night and pre-noon period the N_mF₂ values at both stations are almost equal during the 2 years. However, at post-noon the values at Karachi are considerably larger than those at Islamabad due to the equatorial or geomagnetic anomaly. Karachi (geomag. coord. 16.44°N, 139.08°E) lies near the region of the equatorial anomaly (+20 and −20 geomagnetic latitude), so most of the N_mF₂ values at Karachi are larger than those at Islamabad (geomag. coord. 24.46°N, 145.67°E). The maximum monthly values of N_mF₂ show a semi-annual variation at Karachi and Islamabad both during 1996 and 2000 as predicted by IRI.     

The geomagnetic solar flare effect identified by SIIG as an indicator of a solar flare observed by GOES satellites

This paper studies the efficiency of geomagnetic solar flare effects (gsfe) in X solar flare detection; so during the period 1999–2007 a comparison between solar flare (sf) observed by satellites of the Geostationary Operational Environmental Satellite (GOES) programme and gsfe published by the Service International des Indices Geomagnetiques (SIIG) is made.     

2020年国外惯性技术发展与回顾

通过对IEEE惯性传感器与系统会议、MEMS国际会议、圣彼得堡组合导航会议、PLANS会议和DGON ISS会议等惯性技术相关会议文献,以及惯性技术相关机构发布的一些动态信息进行梳理,总结分析了惯性技术领域的最新发展动态,并重点介绍了光学陀螺、微机电(MEMS)陀螺和加速度计等惯性器件的发展现状,以及美国为增强定位、导...