排序方式: 共有53条查询结果,搜索用时 31 毫秒
31.
Galileo系统完好性处理的方法研究 总被引:1,自引:0,他引:1
对于卫星导航系统而言,系统所能提供的完好性指标和导航定位精度是同样重要的。欧洲的Galileo系统将在2008年建成,届时它将与美国的GPS系统相互补充。本文在对GMileo系统导航定位指标分析的基础上,结合系统完好性监测的设计特点,推导了系统地面完好性信道(GIC)监测算法和用户自主完好性(RAIM)监测算法,建立了数据完好性播发体制。 相似文献
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Mingkui Wu Wanke Liu Renpan Wu Xiaohong Zhang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(7):2003-2020
To ensure the compatibility and interoperability with modernized GPS, Galileo satellites are capable of broadcasting navigation signals on carrier phase frequencies that overlap with GPS, i.e., GPS/Galileo L1-E1/L5-E5a. Moreover, the GPS/Galileo L2-E5b signals have different frequencies with wavelength differences smaller than 4.2?mm. Such overlapping and narrowly spaced signals between GPS and Galileo bring the opportunity to use the tightly combined double-differenced (DD) model for precise real-time kinematic (RTK) positioning, resulting in improved performance of ambiguity resolution and positioning with respect to the classical standard or loosely combined DD model. In this paper, we focus on the model and performance assessment of tightly combined GPS/Galileo L1-E1/L2-E5b/L5-E5a RTK for short and long baselines. We first investigate the tightly combined GPS/Galileo DD observational model for both short and long baselines with simultaneously considering the GPS/Galileo overlapping and non-overlapping frequencies. Particularly, we introduce a reparameterization approach to solve the rank deficiency that caused by the correlation between the DISB parameters and the DD ionospheric parameters for both overlapping and non-overlapping frequencies. Then we present performance assessment for the tightly combined GPS/Galileo RTK model with real-time estimation of the differential inter-system bias (DISB) parameters for short and long baselines in terms of ratio value, ambiguity dilution of precision (ADOP), ambiguity conditional number, decorrelation number, search count, empirical success rate, time-to-first-fix (TTFF), and positioning accuracy. Results from both static and kinematic experiments demonstrated that compared to the loosely combined model, the tightly combined model can deliver improved performance of ambiguity resolution and precise positioning with different satellite visibility. For the car-driven short baseline experiment with 10° elevation cut-off angle, the tightly combined model can not only significantly increase the ratio value by approximately 27.5% (from 16.0 to 20.4), but also reduce the ambiguity ADOP, the conditional number, and the search count in LAMBDA by approximately 22.2% (from 0.027 to 0.021 cycles), 14.9% (from 199.2 to 169.6), and 25.4% (from 150.1 to 112.0), respectively. Comparable decorrelation number, empirical success rate, and positioning accuracy are also obtained. For the car-driven long baseline experiment, it is also observed that the ambiguity resolution performance in terms of the ratio value, the decorrelation number, the condition number, and the search count are significantly improved by approximately 18.5% (from 2.7 to 3.2), 22.0% (from 0.186 to 0.227), 55.9% (from 937.6 to 413.7), and 10.3% (from 43.8 to 39.3), respectively. Moreover, comparable ADOP, empirical success rate, and positioning accuracy are obtained as well. Additionally, the TTFF can be reduced (from 54.1 to 51.8 epochs with 10° elevation cut-off angle) as well from the results of static experiments. 相似文献
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The Galileo E1 open service (OS) and the global positioning system (GPS) L1C are intending to use the multiplexed binary offset carrier (MBOC) modulation in E1/L1 band, including both pilot and data components. The impact of data and pilot codes cross-correlation on the distortion of the discriminator function (i.e., the S-curve) is investigated, when only the pilot (or data) components of MBOC signals are tracked. It is shown that the modulation schemes and the receiver configuration (e.g., the correlator spacing) strongly affect the S-curve bias. In this paper, two methods are proposed to optimize the data/pilot code pairs of Galileo E1 OS and GPS L1C. The optimization goal is to obtain the minimum average S-curve bias when tracking only the pilot components a the specific correlator spacing. Figures of merit, such as S-curve bias, correlation loss and code tracking variance have been adopted for analyzing and comparing the un-optimized and optimized code pairs. Simulation results show that the optimized data/pilot code pairs could significantly mitigate the intra-channel codes cross-correlation, and then improve the code tracking performance of MBOC signals. 相似文献
34.
本文利用轴对称刚体在自身力矩作用下,绕定点运动的一阶正规型运动微分方程代替欧拉方程,讨论航天器的起旋和消旋运动。给出两个卡尔丹角为小量时运动方程的解析积分,由此直接导出航天器相对质心的动量矩矢量及自旋轴在起旋和消旋运动中的变化规律。并以伽里略航天器作为具体对象进行了数值计算。 相似文献
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M. Baguhl E. Grün D. P. Hamilton G. Linkert R. Riemann P. Staubach H. A. Zook 《Space Science Reviews》1995,72(1-2):471-476
Interstellar dust detected by the dust sensor onboard Ulysses was first identified after the Jupiter flyby when the spacecraft's trajectory changed dramatically (Grün et al., 1994). Here we report on two years of Ulysses post-Jupiter data covering the range of ecliptic latitudes from 0° to –54° and distances from 5.4 to 3.2 AU. We find that, over this time period, the flux of interstellar dust particles with a mean mass of 3·10–13 g stays nearly constant at about 1·10–4, m–2 s–1 ( sr)–1, with both ecliptic latitude and heliocentric distance.Also presented are 20 months of measurements from the identical dust sensor onboard the Galileo spacecraft which moved along an in-ecliptic orbit from 1.0 to 4.2 AU. From the impact direction and speeds of the measured dust particles we conclude that Galileo almost certainly sensed interstellar dust outside 2.8 AU; interstellar particles may also account for part of the flux seen between 1 and 2.8 AU. 相似文献
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国外卫星导航定位技术发展现状与趋势 总被引:2,自引:1,他引:1
本报告对目前国外三大卫星导航定位系统GPS ,GLONASS和伽利略系统的技术性能进行了对比研究 ,分析了卫星导航定位技术的未来发展趋势 ,对我国发展卫星导航定位系统提出了建议。 相似文献
40.
S. Dell’Agnello G.O. Delle Monache D.G. Currie R. Vittori C. Cantone M. Garattini A. Boni M. Martini C. Lops N. Intaglietta R. Tauraso D.A. Arnold M.R. Pearlman G. Bianco S. Zerbini M. Maiello S. Berardi L. Porcelli C.O. Alley J.F. McGarry C. Sciarretta V. Luceri T.W. Zagwodzki 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
We built a new experimental apparatus (the “Satellite/lunar laser ranging Characterization Facility”, SCF) and created a new test procedure (the SCF-Test) to characterize and model the detailed thermal behavior and the optical performance of cube corner laser retroreflectors in space for industrial and scientific applications. The primary goal of these innovative tools is to provide critical design and diagnostic capabilities for Satellites Laser Ranging (SLR) to Galileo and other GNSS (Global Navigation Satellite System) constellations. The capability will allow us to optimize the design of GNSS laser retroreflector payloads to maximize ranging efficiency, to improve signal-to-noise conditions in daylight and to provide pre-launch validation of retroreflector performance under laboratory-simulated space conditions. Implementation of new retroreflector designs being studied will help to improve GNSS orbits, which will then increase the accuracy, stability, and distribution of the International Terrestrial Reference Frame (ITRF), to provide better definition of the geocenter (origin) and the scale (length unit). 相似文献