共查询到20条相似文献，搜索用时 15 毫秒
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以卫星双向时间同步算法为基础,分析了运动卫星之间的双向时间同步信号传播延迟随星间距离的变化特点,推导了按此算法计算得到的卫星钟差随星间距离的变化规律,提出了一种利用星间伪距拟合多项式和钟差拟合多项式联合求解高精度星间钟差的卫星动态双向时间同步算法。实际卫星的仿真数据表明,该算法能够把星间的时间同步误差控制在5 ns以内,可用于星间高精度时间同步。 相似文献
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The introduction of an intersatellite link, also called a crosslink, is considered a promising technique for improving the reliability and integrity of a global navigation satellite system. As one of the most rapidly developing satellite navigation systems, the BeiDou system launched from March 2015 to February 2016 an in-orbit validation constellation that includes two inclined geosynchronous orbit satellites and three medium earth orbit satellites equipped with an intersatellite link in the Ka band. We modeled the intersatellite measurements of BeiDou and evaluated the ranging performance of the intersatellite link based on the analysis of in-orbit measurement data. We used both residual analysis and external data comparison to assess the data. The results show that the ranging precision of the BeiDou intersatellite link is within 10 cm and is determined mainly by the thermal noise of the receiver. Moreover, the drift rate of the group delay of the transceiver channel is within 1 cm per day. 相似文献
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B. S. Sheard G. Heinzel K. Danzmann D. A. Shaddock W. M. Klipstein W. M. Folkner 《Journal of Geodesy》2012,86(12):1083-1095
The Gravity Recovery and Climate Experiment (GRACE) has demonstrated that low–low satellite-to-satellite tracking enables monitoring the time variations of the Earth’s gravity field on a global scale, in particular those caused by mass-transport within the hydrosphere. Due to the importance of long-term continued monitoring of the variations of the Earth’s gravitational field and the limited lifetime of GRACE, a follow-on mission is currently planned to be launched in 2017. In order to minimise risk and the time to launch, the follow-on mission will be basically a rebuild of GRACE with microwave ranging as the primary instrument for measuring changes of the intersatellite distance. Laser interferometry has been proposed as a method to achieve improved ranging precision for future GRACE-like missions and is therefore foreseen to be included as demonstrator experiment in the follow-on mission now under development. This paper presents the top-level architecture of an interferometric laser ranging system designed to demonstrate the technology which can also operate in parallel with the microwave ranging system of the GRACE follow-on mission. 相似文献
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北斗广域高精度时间服务原型系统 总被引：1，自引：0，他引：1
基于精密单点定位(precise point positioning,PPP)的时间传递技术以其精度高、覆盖范围广的优点成为性能最优的GNSS时间传递方法之一。随着广域差分产品时效性的提高,实时PPP时间传递开始应用于精密授时的研究。本文在PPP时间传递技术的基础上,结合实时卫星钟差估计、接收机时钟调控及硬件延迟标校技术,建立了基于北斗卫星导航系统(BeiDou navigation satellite system,BDS)的广域高精度时间服务(wide-area precise timing,WPT)系统,可为用户实时提供准确、稳定、可溯源的时间。WPT系统分为时间服务平台和用户终端两个部分。时间服务平台引入高精度的时间作为系统的参考时间基准,并提供广域实时差分改正数;用户终端基于实时PPP时间传递算法获取本地钟与系统时间基准的差异,并采用精密调钟技术实现终端与系统的同步。为了验证系统的实时授时性能,本文进行了零基线、短基线及广域环境下的性能测试和评估。试验结果表明,该系统零基线、短基线时间同步精度优于0.5 ns,广域条件下单天的授时精度均优于1 ns,为基于北斗系统的精密授时技术发展提供了参考。 相似文献
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低轨卫星导航信号增强能够弥补现有中高轨导航卫星信号收敛慢、信号弱的不足,在下一代导航定位技术中占有重要地位。武汉大学研制的珞珈一号科学实验卫星搭载了导航增强载荷,能够在轨自动计算轨道和钟差,并自主生成和播发双频测距信号,首次实现了低轨卫星平台的导航信号增强。就珞珈一号卫星导航增强信号的质量,包括信号载噪比、伪距和载波相位测量精度以及单星授时精度进行了评估,结果显示,珞珈一号卫星高仰角的伪距和载波相位测量精度分别优于1.5 m和1.7 mm,能够满足导航信号增强的需求。珞珈一号卫星单星授时的精度在10~30 ns量级,证明了珞珈一号卫星星地测距链路的正确性和有效性。 相似文献
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地基完好性监测是利用四个或四个以上的精确坐标的监测站对卫星进行监测,计算其星历及星钟误差。该方法需满足四重以上监测站覆盖条件,对于自主导航和区域布站的导航系统不能实现导航卫星的全弧段完好性监测。对于不满足上述覆盖条件的卫星,采用基于星间链路的监测方法,利用四个或四个以上的具有一定坐标误差的卫星对该卫星进行监测。通过星历数据和星间测距数据计算SISMA,从而进行导航卫星全弧段的完好性监测。 相似文献
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A closed-form formula to calculate geometric dilution of precision (GDOP) for multi-GNSS constellations 总被引：2，自引：2，他引：0
With the future global navigation satellite system (GNSS), the multi-GNSS constellations, which are composed of various single systems, will be the main navigation method in future. For the multi-GNSS constellations, the geometric dilution of precision (GDOP) is an important parameter used for satellite selection and the evaluation of positioning accuracy. However, the calculation of GDOP is a time-consuming and power-consuming task. Using Schur complement, we present a closed-form formula to calculate GDOP for multi-GNSS constellations. The formula can be applied to multi-GNSS constellations that include two, three or four different single systems. Furthermore, a closed-form formula for the case of exactly five satellites is also derived. Compared with the conventional numerical methods, the formula can reduce the amounts of multiplication and addition effectively. Numerical experiments validate the effectiveness and feasibility of the closed-form formula. 相似文献
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Analytical derivation of the vegetation optical depth from the microwave polarization difference index 总被引：2，自引：0，他引：2
Meesters A.G.C.A. De Jeu R.A.M. Owe M. 《Geoscience and Remote Sensing Letters, IEEE》2005,2(2):121-123
A numerical solution for the canopy optical depth in an existing microwave-based land surface parameter retrieval model is presented. The optical depth is derived from the microwave polarization difference index and the dielectric constant of the soil. The original procedure used an approximation in the form of a logarithmic decay function to define this relationship and was derived through a series of lengthy polynomials. These polynomials had to be recalculated when the scattering albedo or antenna incidence angle changes. The new procedure is computationally more efficient and accurate. 相似文献
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低低卫-卫跟踪模式中星载KBR系统和GPS接收机指标设计论证 总被引：1，自引：0，他引：1
推导了星载KBR系统的星间距离、星间距离变化率以及星载GPS接收机的卫星轨道位置误差分别影响累计大地水准面精度的误差模型,确定了星载KBR系统和星载GPS接收机的精度指标,建立了星间测速和轨道位置误差联合影响累计大地水准面的误差模型。结果表明,星载KBR系统的星间距离精度指标约为0.64×10-6m,星间距离变化率的精度指标约为0.8×10-6m/s,星载GPS接收机的卫星轨道位置精度指标约为2.1cm。在上述精度指标下,联合误差模型恢复120阶地球重力场对应的累计大地水准面精度约为26cm。 相似文献
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In positioning, navigation and timing applications of multi-GNSS (global navigation satellite system) constellations, the geometric dilution of precision (GDOP) offers an important index for selecting satellites and evaluating positioning accuracy. However, GDOP assumes that the measurement errors of all the tracked satellites are independent and have the same accuracy level, which is impossible in practice, especially when the tracked satellites are from various constellations. Through introducing a weighted matrix describing the measurement errors of different satellites into a common GDOP, we focus on new characteristics of weighted GDOP (WGDOP) in two aspects. First, we compare the sizes of WGDOP and the common GDOP based on the range of the weights of different satellites, i.e., the diagonal elements of the weighted matrix. In addition, when the weights of different satellites increase, the change of WGDOP with the weights is also derived. Moreover, a closed-form formula for calculating WGDOP is also presented. The theoretical derivations demonstrate that the closed-form can reduce the computation burden effectively. Furthermore, numerical tests verify these analyses. 相似文献
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Satellite clock bias estimation for iGPS 总被引：4，自引：0，他引：4
John Pratt Penina Axelrad Kristine M. Larson Bruno Lesage Richard Gerren Nicholas DiOrio 《GPS Solutions》2013,17(3):381-389
The High Integrity GPS program seeks to provide enhanced navigation performance by combining conventional GPS with a communications and ranging broadcast from the Iridium® Communications System. Through clock and message aiding, it would enable existing GPS receivers to acquire and track in more challenging environments. As is the case for standard GPS, accurate and precise timing is key to performance. An approach is presented for estimating the bias of each Iridium satellite clock using satellite-to-ground and satellite-to-satellite measurements. The satellite clock bias estimates are based on a Kalman filter that incorporates code-type observations from the measurements at 10 s intervals. Filter parameters are set based on the expected behavior of the clocks, allowing for discontinuous bias and frequency adjustments due to ground commands. Typical results show the current filter to be accurate to within 200 ns while always meeting the initial system specification of half a microsecond. 相似文献
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本文在仿真出GPS系统与BDS系统卫星星座的基础上,对两种定位系统下的哈尔滨、武汉、广州、拉萨单个站点以及全球范围的卫星可见性、DOP值、定位精度进行了覆盖分析,并比较了两个系统定位性能的差异。实验结果表明,当前BDS系统在亚太地区与GPS系统的定位性能基本一致,可见卫星数比GPS系统稍多,但BDS系统的DOP值的波动却比GPS系统的要大,尤其在GEO与IGSO卫星覆盖的边缘区域,BDS的导航定位性能较差,在某些地区仍不能提供导航定位服务。 相似文献
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气象卫星发展回顾与展望 总被引：1，自引：0，他引：1
回顾了国际气象卫星和中国风云气象卫星的发展,综述了气象卫星在图像解译、定量产品应用和数据同化方面的成就以及辐射校正技术的进步。围绕大气科学,特别是数值天气预报对天基观测的需求,展望了未来气象卫星的技术发展方向。 相似文献
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提出了一种基于GPS的多站实时时间传递算法,该算法将卫星钟差作为未知参数进行实时估计,利用测站间的共视卫星建立起各测站误差方程之间的联系,同时解算站间时间传递结果和卫星钟差。摆脱了对外部事后精密卫星钟差产品的依赖,不受卫星精密钟差产品精度和实时性的限制,只要站间有足够的共视卫星,即可实现时间传递。实验结果表明:该算法时间传递精度可以达到亚纳秒量级,能够应用于高精度实时时间传递。 相似文献
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Simulation study of a follow-on gravity mission to GRACE 总被引：9，自引：3，他引：6
The gravity recovery and climate experiment (GRACE) has been providing monthly estimates of the Earth’s time-variable gravity
field since its launch in March 2002. The GRACE gravity estimates are used to study temporal mass variations on global and
regional scales, which are largely caused by a redistribution of water mass in the Earth system. The accuracy of the GRACE
gravity fields are primarily limited by the satellite-to-satellite range-rate measurement noise, accelerometer errors, attitude
errors, orbit errors, and temporal aliasing caused by un-modeled high-frequency variations in the gravity signal. Recent work
by Ball Aerospace & Technologies Corp., Boulder, CO has resulted in the successful development of an interferometric laser
ranging system to specifically address the limitations of the K-band microwave ranging system that provides the satellite-to-satellite
measurements for the GRACE mission. Full numerical simulations are performed for several possible configurations of a GRACE
Follow-On (GFO) mission to determine if a future satellite gravity recovery mission equipped with a laser ranging system will
provide better estimates of time-variable gravity, thus benefiting many areas of Earth systems research. The laser ranging
system improves the range-rate measurement precision to ~0.6 nm/s as compared to ~0.2 μm/s for the GRACE K-band microwave
ranging instrument. Four different mission scenarios are simulated to investigate the effect of the better instrument at two
different altitudes. The first pair of simulated missions is flown at GRACE altitude (~480 km) assuming on-board accelerometers
with the same noise characteristics as those currently used for GRACE. The second pair of missions is flown at an altitude
of ~250 km which requires a drag-free system to prevent satellite re-entry. In addition to allowing a lower satellite altitude,
the drag-free system also reduces the errors associated with the accelerometer. All simulated mission scenarios assume a two
satellite co-orbiting pair similar to GRACE in a near-polar, near-circular orbit. A method for local time variable gravity
recovery through mass concentration blocks (mascons) is used to form simulated gravity estimates for Greenland and the Amazon
region for three GFO configurations and GRACE. Simulation results show that the increased precision of the laser does not
improve gravity estimation when flown with on-board accelerometers at the same altitude and spacecraft separation as GRACE,
even when time-varying background models are not included. This study also shows that only modest improvement is realized
for the best-case scenario (laser, low-altitude, drag-free) as compared to GRACE due to temporal aliasing errors. These errors
are caused by high-frequency variations in the hydrology signal and imperfections in the atmospheric, oceanographic, and tidal
models which are used to remove unwanted signal. This work concludes that applying the updated technologies alone will not
immediately advance the accuracy of the gravity estimates. If the scientific objectives of a GFO mission require more accurate
gravity estimates, then future work should focus on improvements in the geophysical models, and ways in which the mission
design or data processing could reduce the effects of temporal aliasing. 相似文献