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1.
Wenwu Ding Bingfeng Tan Yongchang Chen Felix Norman Teferle Yunbin Yuan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(3):951-961
The performance of real-time (RT) precise positioning can be improved by utilizing observations from multiple Global Navigation Satellite Systems (GNSS) instead of one particular system. Since the end of 2012, BeiDou, independently established by China, began to provide operational services for users in the Asia-Pacific regions. In this study, a regional RT precise positioning system is developed to evaluate the performance of GPS/BeiDou observations in Australia in providing high precision positioning services for users. Fixing three hourly updated satellite orbits, RT correction messages are generated and broadcasted by processing RT observation/navigation data streams from the national network of GNSS Continuously Operating Reference Stations in Australia (AUSCORS) at the server side. At the user side, RT PPP is realized by processing RT data streams and the RT correction messages received. RT clock offsets, for which the accuracy reached 0.07 and 0.28?ns for GPS and BeiDou, respectively, can be determined. Based on these corrections, an accuracy of 12.2, 30.0 and 45.6?cm in the North, East and Up directions was achieved for the BeiDou-only solution after 30 min while the GPS-only solution reached 5.1, 15.3 and 15.5?cm for the same components at the same time. A further improvement of 43.7, 36.9 and 45.0 percent in the three directions, respectively, was achieved for the combined GPS/BeiDou solution. After the initialization process, the North, East and Up positioning accuracies were 5.2, 8.1 and 17.8?cm, respectively, for the BeiDou-only solution, while 1.5, 3.0, and 4.7?cm for the GPS-only solution. However, we only noticed a 20.9% improvement in the East direction was obtained for the GPS/BeiDou solution, while no improvements in the other directions were detected. It is expected that such improvements may become bigger with the increasing accuracy of the BeiDou-only solution. 相似文献
2.
通过对比北斗卫星导航系统(BeiDou Navigation Satellite System,BDS)广播星历与事后精密星历,提取了轨道和卫星时钟误差。基于北斗轨道误差及北斗卫星时钟误差统计特征分析,构建区别于全球定位系统(Global Positioning System,GPS)的BDS空间信号用户测距误差(Signal-In-Space User Range Error,SISRE)描述方法,对BDS广播星历中用户测距精度(User Range Accuracy,URA)进行了验证。6个月的北斗数据测试结果表明,北斗GEO、IGSO和MEO卫星的URA分别为3.0m、1.9m和1.6m。 相似文献
3.
由于在复杂FPGA(Field Programmable Gate Array,现场可编程门阵列)设计中存在跨时钟域,通常会产生亚稳态现象.为有效地预防和解决该问题,分析FPGA设计中亚稳态的产生机理及其对数字信号处理系统的影响.根据不同的信号同步类型,针对单比特电平信号、脉冲信号和边沿信号,分别给出基于触发器级联的跨时钟域信号同步方法;针对并行信号,提出基于异步FIFO (First In First Out,先进先出队列)和握手协议的跨时钟域同步方法;并通过仿真手段分析信号同步方法的有效性及其适用范围.结果表明:这些方法能够正确有效地完成跨时钟域信号同步,预防可能出现的亚稳态问题,从而提高复杂FPGA设计的可靠性和稳定性. 相似文献
4.
针对北斗卫星导航系统(BDS)钟差预报产品无法满足高精度快速服务需求的现状,提出了一种基于BDS-2/BDS-3联合估计的超快速卫星钟差预报优化策略。区别于传统两步法预报模型,利用稀疏建模方法一步求解所有模型项,并通过BDS-2/BDS-3星间相关性实现了模型系数解的增强;为进一步降低模型残差的影响,基于残差序列时空相关性,利用半变异函数重构了模型估计的权阵。为验证提出的钟差预报模型,设计了12套对比方案,实验结果表明:基于稀疏建模的钟差模型参数一步估计可略微提高钟差预报精度;通过引入星间相关性对随机模型进行精化,钟差序列一步建模可分别将BDS-2与BDS-3卫星钟差18h预报精度提升28.6%与27.2%;基于半变异函数建模的模型残差相关性提取,可实现BDS-2与BDS-3预报钟差精度8.0%与11.1%的提升。因此,提出的优化策略对当前北斗超快速卫星钟差预报产品精化具有重要意义。 相似文献
5.
6.
提出一种面向未来卫星在轨应用的闭环物理高精度时间同步方法。比较了所提方法与其他时间同步方法的区别与优势,建立了远程系统时间同步基本模型与误差传递模型,基于双向测距和时间传递技术分析了高精度钟差获取原理,给出了时钟调整环路的时域频域参数依赖关系。完成了高精度时间同步地面试验系统构建,测试了开环非调钟状态下钟差测量精度误差、闭环调钟状态下时间同步准确度误差以及长时运行情况下的时间同步监测结果。测试结果表明,该方法能够实现优于1 ns量级的时间同步,为高精度时间同步技术研究提供了新的途径。 相似文献
7.
8.
Haykel Elabidi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We present in this work energy levels, oscillator strengths, radiative decay rates and fine structure collision strengths for the Mg III and Al IV ions. The 11 configurations: (1s2) 2s22p6, 2s22p53l, 2s2p63l, 2s22p54l (l?n-1, where n is the principal quantum number), yielding the lowest 75 levels are used. The collisional data for these two ions are missing in the literature, especially the database CHIANTI, this is the principal motivation behind the present work. Calculations have been performed using the AUTOSTRUCTURE code. AUTOSTRUCTURE treats the scattering problem in the distorted wave approach. Fine structure collision strengths are calculated for a range of electron energies from 10 Ry to 240 Ry. The atomic structure data are compared to available experimental and theoretical results. 相似文献
9.
R. Stamm R. Hammami I. Hannachi H. Capes L. Godbert-Mouret M. Koubiti Y. Marandet J. Rosato 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Stochastic processes provide flexible and fast calculations for modeling dynamical interactions between an atom and charged particles. We use a stochastic renewal process for the plasma microfield being the cause of Stark broadening. The accuracy and improvement possibilities of Lyman profiles calculations with a renewal process are analyzed by comparing to ab initio simulations for ion broadening only. Stochastic processes may also be applied to out of equilibrium plasmas. We present our first results for the effect of Langmuir waves on a line broadened by electrons only, and for the changes of atomic populations submitted to strong temperature fluctuations. 相似文献
10.
F. Ramírez-Martínez C. Lacroûte P. Rosenbusch F. Reinhard C. Deutsch T. Schneider J. Reichel 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
We present a compact atomic frequency standard based on the interrogation of magnetically trapped 87Rb atoms. Two photons, in the microwave and radiofrequency domain excite the atomic transition. At a magnetic field of 3.23 G this transition from ∣F = 1, mF = −1〉 to ∣F = 2, mF = 1〉 is 1st order insensitive to magnetic field variations. Long Ramsey interrogation times can thus be achieved, leading to a projected stability in the low 10−13 at 1 s. This makes this device a viable alternative to LITE and HORACE as a good candidate for replacing or complementing the rubidium frequency standards and passive hydrogen masers already on board of the GPS, GLONASS, and GALILEO satellites. Here we present preliminary results. We use an atom chip to cool and trap the atoms. A coplanar waveguide is integrated to the chip to carry the Ramsey interrogation signal, making the physics package potentially as small as (5 cm)3. We describe the experimental apparatus and show preliminary Ramsey fringes of 1.25 Hz linewidth. We also show a preliminary frequency stability σy = 1.5 × 10−12τ−1/2 for 10 < τ < 103 s. This represents one order of magnitude improvement with respect to previous experiments. 相似文献