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基于IGS超快速星历的高精度实时GPS测量 总被引：1，自引：0，他引：1
IGS的几种星历产品中,精密星历精度虽然高,但不能实时获得,并且它是影响高精度实时测量应用的主要因素。讨论几种星历产品数值上的差异,在实际计算中使用超快预报星历替代精密星历,并比较它们基线解算结果和天顶延迟解算结果。结果证明：两种星历计算的基线差别非常小,因此,在高精度GPS数据处理中可以直接使用超快预报星历,得到高精度的实时坐标。同样可以应用在GPS气象中,用超快事后星历实现对流层实时监测。 相似文献
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卫星钟差的难预测性是影响实时高精度定位的重要因素之一。为快速获得高精度位置或对流层等信息,在非差观测模型的基础上,本文提出了一种延迟量约1 h的近实时钟差估计策略,该策略主要包含超快速轨道解算和钟差估计两部分。经验证,预报部分第2~5 h的GPS轨道三维平均精度为3.85 cm,BDS GEO和IGSO+MEO轨道三维平均精度分别为81.4和21.74 cm。基于超快速轨道可获得近实时钟差精度GPS为0.054 ns,BDS为0.12 ns。最后通过BDS+GPS静态PPP试验验证了轨道和钟差的可用性。 相似文献
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The International GNSS Service (IGS) issues four sets of so-called ultra-rapid products per day, which are based on the contributions of the IGS Analysis Centers. The traditional (“old”) ultra-rapid orbit and earth rotation parameters (ERP) solution of the Center for Orbit Determination in Europe (CODE) was based on the output of three consecutive 3-day long-arc rapid solutions. Information from the IERS Bulletin A was required to generate the predicted part of the old CODE ultra-rapid product. The current (“new”) product, activated in November 2013, is based on the output of exactly one multi-day solution. A priori information from the IERS Bulletin A is no longer required for generating and predicting the orbits and ERPs. This article discusses the transition from the old to the new CODE ultra-rapid orbit and ERP products and the associated improvement in reliability and performance. All solutions used in this article were generated with the development version of the Bernese GNSS Software. The package was slightly extended to meet the needs of the new CODE ultra-rapid generation. 相似文献
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研究了基线解算时分别使用广播星历、快速星历和精密星历时解算结果的影响.对于长基线来讲,使用快速星历和精密星历可以有效提高解算精度,对于短基线,使用广播星历可以保证基线解算的精度. 相似文献
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We present earth rotation results from the ultra-rapid operations during the continuous VLBI campaigns CONT11 and CONT14. The baseline Onsala–Tsukuba, i.e., using two out of the 13 and 17 stations contributing to CONT11 and CONT14, respectively, was used to derive UT1-UTC in ultra-rapid mode during the ongoing campaigns. The latency between a new observation and a new UT1-UTC result was less than 10 min for more than 95% of the observations. The accuracy of the derived ultra-rapid UT1-UTC results is approximately a factor of three worse than results from optimized one-baseline sessions and/or complete analysis of large VLBI networks. This is, however, due to that the one-baseline picked from the CONT campaigns is not optimized for earth rotation determination. Our results prove that the 24/7 operation mode planned for VGOS, the next-generation VLBI system, is possible already today. However, further improvements in data connectivity of stations and correlators as well in the automated analysis are necessary to realize the ambitious VGOS plans. 相似文献
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IGS超快速星历预推GPS卫星轨道精度分析 总被引：1，自引：0，他引：1
在GPS卫星星历中,除了GPS广播星历能被GPS用户实时获取进行实时定位和导航外,IGS超快速星历(IGU星历)有24 h的预推轨道也能被GPS用户实时得到,可以利用IGU星历的预推轨道进行实时定位和导航。文中对IGS发布的IGS超快速星历(IGU星历)预推轨道精度进行了分析。研究表明,随着IGU发布的频度提高,其预推轨道精度也进一步提高,对于每天发布4次的IGU星历,预推轨道的前6 h轨道精度在X、Y、Z方向分别为3.2 cm3、.4 cm、3.2 cm。 相似文献
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Maintaining real-time precise point positioning during outages of orbit and clock corrections 总被引：1，自引：1，他引：0
The precise point positioning (PPP) is a popular positioning technique that is dependent on the use of precise orbits and clock corrections. One serious problem for real-time PPP applications such as natural hazard early warning systems and hydrographic surveying is when a sudden communication break takes place resulting in a discontinuity in receiving these orbit and clock corrections for a period that may extend from a few minutes to hours. A method is presented to maintain real-time PPP with 3D accuracy less than a decimeter when such a break takes place. We focus on the open-access International GNSS Service (IGS) real-time service (RTS) products and propose predicting the precise orbit and clock corrections as time series. For a short corrections outage of a few minutes, we predict the IGS-RTS orbits using a high-order polynomial, and for longer outages up to 3 h, the most recent IGS ultra-rapid orbits are used. The IGS-RTS clock corrections are predicted using a second-order polynomial and sinusoidal terms. The model parameters are estimated sequentially using a sliding time window such that they are available when needed. The prediction model of the clock correction is built based on the analysis of their properties, including their temporal behavior and stability. Evaluation of the proposed method in static and kinematic testing shows that positioning precision of less than 10 cm can be maintained for up to 2 h after the break. When PPP re-initialization is needed during the break, the solution convergence time increases; however, positioning precision remains less than a decimeter after convergence. 相似文献
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There are three aspects in the study of GPS meteorology network in the Wuhan region. The first is the comparison of the GPS precipitable water vapor between final ephemeris and ultra-rapid ephemeris for which the relative coefficient is 99.97 and the root mean squares is 0.048 mm. It can be concluded that ultra-rapid ephemeris can be used to get the GPS precipitable water vapor for the real-time prediction. The second is the comparison of precipitable water vapor of GPS stations and the distribution of water vapor in the Wuhan region is acquired. The change of GPS precipitable water vapor and rainfall in a rainfall process are compared and analyzed. The change of GPS precipitable water vapor can reflect and predict the process of rainfall. 相似文献
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GPS实时精密单点定位需要实时的、精确的、可靠的预报卫星钟差预报,因此卫星钟差的预报是一项非常重要的工作,它对实时的高精度导航定位具有重要意义。为导航定位提供时间标准的导航卫星原子钟是非常精密的仪器,对外界环境非常敏感,无法将卫星钟差作为普通的白噪声处理,可以但可将卫星钟差看作是灰色系统来进行研究。本文根据灰色系统相关理论,将灰色系统模型GM(1,1)应用到卫星钟差的预报,并用IGS超快速星历建立了预报卫星钟差的灰色预测模型,研究了卫星钟差的变化规律。结果表明:灰色模型可用于卫星钟差的短期预报,它对超快速星历的预报精度与IGS产品中的IGU超快速星历本身的预报精度相当。 相似文献
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武汉地区GPS气象网试验研究 总被引：1，自引：1，他引：1
将精密星历与快速预报星历GPS可降水量进行比较，两者的相关系数为99．97％，均方根为0．048mm，得出可以利用快速预报星历进行GPS可降水量的准实时预报的结论。通过对武汉地区GPS测站的可降水量的比较，得出武汉地区水汽的分布状况。对一次降雨过程进行了GPS可降水量与实际降雨量的比较，表明GPS可降水量变化可反映和预报降雨发生的过程。 相似文献
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针对IGS超快星历钟差预报产品(IGU-P)精度较低及无法满足高精度实时PPP定位精度的问题,提出了一种GPS IIR-M型卫星超快星历钟差预报的高精度修正方法。该方法对预报值的第一个数据与IGU观测部分(IGU-O)数据的最后一个历元做差,根据差值对整个IGU-O差分序列的影响程度来确定精度修正的大小和方向,从而实现IIR-M型卫星高精度预报的效果。经过IGU实测数据的测试结果表明,在短期预报6 h范围内,本文提出的精度修正方法可使3种预报方案在原有预报精度基础上分别提升6.13%、3.9%和3。48%,预报精度分别控制在0.599 ns、0.570 ns和0.531 ns,且均优于IGU-P产品预报精度。 相似文献
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在实时GPS精密单点定位中,能否快速有效地得到高精度的卫星钟差预报值是影响实时单点定位速度和精度的一个重要因素,由于GPS原子钟的高频率、高敏感和极易受到外界及其本身因素影响的性质使得卫星钟差预报至今都没能得到很好地解决,本文在目前的卫星钟差预报基础上,分别探讨了利用灰色模型理论、线性模型和二次多项式模型等方法,以IGS超快星历中2004年12月7日卫星钟差观测资料预报8日的卫星钟差为例进行卫星钟差预报研究,初步得出如下结论:在利用IGS超快星历的前一天的卫星钟差观测值预报后一天的钟差时,线性模型相对方便有效;而灰色模型只要选取合适的模型指数系数,能得到较高精度;但二次多项式模型预报精度较差。利用线性模型能达到或优于IGS超快星历预报钟差的预报精度。 相似文献
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Different types of GPS clock and orbit data provided by the International GPS Service (IGS) have been used to assess the accuracy
of rapid orbit determination for satellites in low Earth orbit (LEO) using spaceborne GPS measurements. To avoid the need
for reference measurements from ground-based reference receivers, the analysis is based on an undifferenced processing of
GPS code and carrier-phase measurements. Special attention is therefore given to the quality of GPS clock data that directly
affects the resulting orbit determination accuracy. Interpolation of clock data from the available 15 min grid points is identified
as a limiting factor in the use of IGS ultra-rapid ephemerides. Despite this restriction, a 10-cm orbit determination accuracy
can be obtained with these products data as demonstrated for the GRACE-B spacecraft during selected data arcs between 2002
and 2004. This performance may be compared with a 5-cm orbit determination accuracy achievable with IGS rapid and final products
using 5 min clock samples. For improved accuracy, high-rate (30 s) clock solutions are recommended that are presently only
available from individual IGS centers. Likewise, a reduced latency and more frequent updates of IGS ultra-rapid ephemerides
are desirable to meet the requirements of upcoming satellite missions for near real-time and precise orbit determination. 相似文献
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实时获取高时空分辨率的大气水汽是制约数值天气预报准确性的关键问题。基于地基GPS遥感大气水汽原理,结合香港CORS网的实测数据进行处理,对由IGU超快速星历、IGS精密星历和探空资料解算的大气可降水量(Precipitable Water Vapor,PWV)序列进行比较分析。实验结果表明,利用超快速星历估计PWV用于数值天气预报是切实可行的。 相似文献
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网络RTK是利用多基准站观测值实现流动站附近的误差建模,其中包括对流层、电离层延迟和卫星轨道等误差。讨论了利用VRS技术实现网络RTK中的几个关键技术,包括将多基准站插值所得的双差大气延迟添加到非差模式的VRS观测值中,利用IGS的超快速星历中的预报部分改正广播星历误差和利用恒星日滤波改正VRS的伪距多路径效应。24 ... 相似文献
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