共查询到20条相似文献，搜索用时 140 毫秒
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我国的北斗系统（BDS）是目前唯一全系统卫星播发三频信号并能提供区域成熟导航定位服务的卫星定位系统。相比双频信号,利用三频信号有望获得更好的导航定位结果。本文基于实测BDS三频数据,主要测试分析了双频消电离层组合和三频模式下的最小噪声消电离层组合的伪距差分定位性能。首先利用历元间观测值差分的方法,获取了实测BDS数据3个频点的伪距精度;其次应用最小范数法求解了三频最小噪声消电离层组合系数。理论分析结果表明,三频伪距噪声最优组合相比双频情况有所改进,但幅度不大;基于实测北斗三频数据的定位结果也显示出相同的结论,即定位精度略有提升,但幅度不大。 相似文献
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针对北斗三号新的三频观测值,通过分析BDS-3三频线性组合观测值特性,选取高质量组合观测值,采用无几何相关GF(Geometry-Free)模型和无几何无电离层相关GIF(Geometry-Ionospheric-Free)模型分别对实测BDS-3卫星数据进行单历元三频相位模糊度解算TCAR(Triple-freque... 相似文献
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基于北斗三频的短基线单历元模糊度固定 总被引：2，自引：0，他引：2
采用三频观测值能组成更多波长更长、噪声较小的观测值;通过依次固定超宽巷、宽巷、窄巷模糊度,可以实现模糊度的快速固定。目前以TCAR、CIR为代表的方法均是基于无几何模型的方法,通过伪距直接求解相位模糊度;由于不同卫星模糊度各自单独求解,没有综合利用所有卫星的观测值信息。基于有几何模型,使用LAMBDA方法进行逐级模糊度固定,依次固定超宽巷、两个宽巷、两个无电离层组合窄巷模糊度,最后使用模糊度固定的两个无电离层组合进行最终基线解算。北斗实测数据验证表明,针对10km的短基线数据,采用本文方法可以实现100%的单历元模糊度固定的成功率。 相似文献
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《测绘工程》2020,(2)
针对载波相位观测值中出现周跳的问题及北斗三号系统(BDS-3)将至少有B_(1I),B_(1C),B_(2a)和B_(3I) 4个信号提供全球公开服务的现状,研究北斗三号系统的周跳探测与修复。提出优化三频相位电离层残差二阶历元差分组合和三频无几何无电离层相位组合的信号排列顺序,可进一步削弱组合观测量的电离层延迟影响和噪声影响,并基于北斗三号的实测数据,联合STPIR法、MW法和无几何无电离层相位组合法进行周跳探测与修复实验。实验结果表明,组合观测量信号的优化排列,削弱组合观测量的电离层延迟影响和噪声影响,且所选的3个组合观测量可以准确探测所有周跳,并有效地修复。 相似文献
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电离层折射误差是卫星导航系统定位的主要误差源之一。目前使用最广泛、最有效的电离层折射误差改正技术是双频技术。区域卫星导航系统具有3个频率的观测数据,可以形成多种消除电离层一阶项的观测组合以及消除电离层二阶项的观测数据。文中假设各个频率上的观测噪声相同,推导了B1/B2,B1/B3和B2/B3三种消电离层一阶项组合的表达式,其噪声放大因子分别为2.899,3.527和14.286;推导了B1/B2/B3消电离层一阶项且噪声最小组合的表达式,组合系数分别为6.179,-3.826和-1.000,该组合的噪声放大因子为2.865;推导了消除电离层二阶项组合的表达式,组合系数分别为-0.263,-0.749和1.000,该组合的噪声放大因子为35.748。利用实测的伪距数据对5种组合的定位误差进行了计算。定位结果表明,消电离层一阶项且噪声最小的定位精度最高;B1/B2,B1/B3和B2/B3组合定位精度依次降低;B1/B2/B3消电离层二阶项组合虽然消除了电离层二阶项,但噪声放大了35.748倍,因此其定位精度最差。 相似文献
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针对历元间隔较大或电离层延迟较大的情况,采用两个无几何相位组合与一个最优无几何无电离层组合形成3个线性无关的探测量,将历元间高次差法引用到无几何相位组合探测量中,通过选取合适的探测阈值,使无几何相位组合能够正确探测到较大电离层影响情况下的不敏感周跳。此外,文中采用了一种特殊的无几何无电离组合观测量进行辅助修复,通过两次取整保证了周跳修复的准确性,避免了传统三频周处理中的搜索算法造成错误修复的问题,试验表明,文中算法可以正确探测与修复较大电离层影响情况下不同北斗卫星星座类型的所有小周跳组合以及不敏感周跳组合。 相似文献
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为了进一步分析北斗卫星观测值的相关特性,文章对比北斗卫星与GPS卫星、以及不同类型北斗卫星之间观测值特性的差异,提出了用站间差分考察伪距多路径组合和GFIF组合观测值的方法。陆态网络数据实验结果显示,北斗卫星B1频率观测值的信噪比最低;高度角较低时,北斗卫星伪距多路径组合绝对值和离散度均较大,约为1.5m,且IGSO和MEO卫星的伪距多路径组合值随高度角增大而明显降低;北斗GEO和IGSO卫星的相位GFIF组合有日周期性,变化范围约为±2cm,伪距GFIF组合的变化范围可达±2m;站间差分可明显减弱伪距多路径组合的变化趋势和相位GFIF组合的周期性,表明这两个组合中可能包含与卫星相关的误差,为北斗观测数据误差处理提供参考。 相似文献
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利用码和载波相位观测值半和线性组合可以消除电离层一阶误差的特性,讨论了基于UofC消电离层组合的GPS/GLONASS精密单点定位的数学模型。UofC模型对两个频率上的模糊度参数分别进行估计,为进一步获得模糊度参数的整数解提供了便利。利用IGS跟踪站的GPS/GLONASS观测数据对UofC模型和传统的在两个频率码观测值间进行消电离层组合的模型进行了比较,统计结果表明,UofC模型与传统模型相比在平面位置定位精度上略有提高,但总体上差别不大。 相似文献
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This study analyzes the quality of onboard data of tracking signals from GPS satellites on the far side of the earth and determines the orbit of the geostationary satellite using code and carrier phase observations with 30-h and 3-day orbit arc length. According to the analysis results, the onboard receiver can track 6–8 GPS satellites, and the minimum and maximum carrier to noise spectral densities were 24 and 45 dB-Hz, respectively. For a GPS receiver on a high-altitude platform above the navigation constellations, the blocking of the earth and a weak signal strength usually cause a piece-wise GPS signal tracking and an increase in the number of ambiguity parameters. Individual GPS satellites may be continuously tracked for as little as several minutes and as long as 3 h. Moreover, considering the negative sign of elevation angles reflects the fact that GPS satellites are tracked below the receiver in the study. GPS satellites appear mainly in the elevation angle range of ??53° to ??83°, and dilution of precision values could reach ten or one hundred and more. Also, it is observed that when a signal suffers from atmospheric refraction, other GPS signals tracked simultaneously by the receiver experience strong systematic errors in the code observations. Based on single-frequency code and carrier phase measurements, the mean 3D root mean square (RMS) value of the overlap comparisons between 30-h orbit determination arcs is 2.14 m. However, we found that there were also some biases in the carrier phase residuals, which contributed to poor orbit accuracy. To eliminate the effects of the biases, we established a correction sequence for each GPS satellite. After corrections, the mean 3D RMS was reduced to 0.99 m, representing a 53% improvement. 相似文献
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Ambiguity resolution for triple-frequency geometry-free and ionosphere-free combination tested with real data 总被引：5，自引：3，他引：2
The recent GPS Block IIF satellites SVN62 and SVN63 and the Galileo satellites GIOVE-A, GIOVE-B, PFM and FM2 already send signals on more than two frequencies, and more GNSS satellites will provide tracking data on at least three frequencies in the near future. In this paper, a simplified general method for ambiguity resolution minimizing the noise level for the triple-frequency geometry-free (GF) and ionosphere-free (IF) linear combinations is presented, where differently scaled code noise on the three frequencies was introduced. For the third of three required linear combinations, the most demanding one in triple-frequency ambiguity resolution, we developed a general method using the ambiguity-corrected phase observations without any constraints to search for the optimal GF and IF linear combination. We analytically demonstrate that the noise level of this third linear combination only depends on the three frequencies. The investigation concerning this frequency-dependent noise factor was performed for GPS, Galileo and Compass frequency triplets. We verified the theoretical derivations with real triple-frequency GPS and Galileo data from the Multi-GNSS Experiment (M–GEX) of the International GNSS Service (IGS). The data of about 30 M–GEX stations around the world over 11 days from 29 April 2012 to 9 May 2012 were used for the test. For the third linear combinaton using Galileo E1, E5b and E5a, which is expected to have the worst performance among all the GNSS frequency triplets in our investigation, the formal errors of the estimated ambiguities are in most cases below 0.2 cycles after 400 observation epochs. If more GPS satellites sending signals on three frequencies or more stations tracking Galileo E6 signal are available in the future, an improvement by a factor of two to three can be expected. 相似文献
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区域卫星导航系统GEO卫星定轨观测模型 总被引：1，自引：0，他引：1
根据GEO导航卫星的轨道特性，给出了数学上严密的卫星伪距观测和载波相位观测模型，讨论了GEO卫星轨道和卫星钟差的解算条件以及单星定轨、多星组差定轨的可行性。 相似文献
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Xiaohong Zhang Mingkui Wu Wanke Liu Xingxing Li Shun Yu Cuixian Lu Jens Wickert 《Journal of Geodesy》2017,91(10):1225-1240
The successful launch of five new-generation experimental satellites of the China’s BeiDou Navigation Satellite System, namely BeiDou I1-S, I2-S, M1-S, M2-S, and M3-S, marks a significant step in expanding BeiDou into a navigation system with global coverage. In addition to B1I (1561.098 MHz) and B3I (1269.520 MHz) signals, the new-generation BeiDou-3 experimental satellites are also capable of transmitting several new navigation signals in space, namely B1C at 1575.42 MHz, B2a at 1176.45 MHz, and B2b at 1207.14 MHz. For the first time, we present an initial characterization and performance assessment for these new-generation BeiDou-3 satellites and their signals. The L1/L2/L5 signals from GPS Block IIF satellites, E1/E5a/E5b signals from Galileo satellites, and B1I/B2I/B3I signals from BeiDou-2 satellites are also evaluated for comparison. The characteristics of the B1C, B1I, B2a, B2b, and B3I signals are evaluated in terms of observed carrier-to-noise density ratio, pseudorange multipath and noise, triple-frequency carrier-phase ionosphere-free and geometry-free combination, and double-differenced carrier-phase and code residuals. The results demonstrate that the observational quality of the new-generation BeiDou-3 signals is comparable to that of GPS L1/L2/L5 and Galileo E1/E5a/E5b signals. However, the analysis of code multipath shows that the elevation-dependent code biases, which have been previously identified to exist in the code observations of the BeiDou-2 satellites, seem to be not obvious for all the available signals of the new-generation BeiDou-3 satellites. This will significantly benefit precise applications that resolve wide-lane ambiguity based on Hatch–Melbourne–Wübbena linear combinations and other applications such as single-frequency precise point positioning (PPP) based on the ionosphere-free code–carrier combinations. Furthermore, with regard to the triple-frequency carrier-phase ionosphere-free and geometry-free combination, it is found that different from the BeiDou-2 and GPS Block IIF satellites, no apparent bias variations could be observed in all the new-generation BeiDou-3 experimental satellites, which shows a good consistency of the new-generation BeiDou-3 signals. The absence of such triple-frequency biases simplifies the potential processing of multi-frequency PPP using observations from the new-generation BeiDou-3 satellites. Finally, the precise relative positioning results indicate that the additional observations from the new-generation BeiDou-3 satellites can improve ambiguity resolution performance with respect to BeiDou-2 only positioning, which indicates that observations from the new-generation BeiDou-3 satellites can contribute to precise relative positioning. 相似文献
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GPS／GLONASS载波相位测量模糊度解算方法 总被引：3，自引：1，他引：3
GPS／GLONASS组合载波相位测量，在快速静态和动态定位等方面的应用具有一定的优势。由于GLONASS采用频分多址的方式识别卫星，每颗卫星的载波频率各不相同，所以在载波测量数据处理中不能采用与GPS载波相位测量数据处理相同的方法。文中就GLONASS、GPS／GLONASS组合载波相位测量整周模糊度解算的基本思路和方法进行了介绍。 相似文献
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X. X. Jin 《Journal of Geodesy》1997,71(7):411-422
This paper derives a DGPS positioning algorithm, referred to as the algorithm for carrier-adjusted DGPS positioning. This
algorithm can be applied by a DGPS user when code and carrier observations are available and when the dynamic behaviours of
both mobile positions and receiver-clock biases can and cannot be modelled. Since the algorithm directly uses code and carrier
observations, the stochastic model of observations has a simple structure and can be easily specified. When the dynamic behaviour
of mobile positions can be modelled, the algorithm can provide recursive solutions of the positions, on the other hand, when
the behaviour cannot be modelled, it can provide their instantaneous solutions. Furthermore, the algorithm can integrate with
a real-time quality-control procedure so that the quality of the position estimates can be guaranteed with a certain probability.
Since in the use of the algorithm there always exist redundant observations unless the position parameters are inestimable,
the quality control can even be performed when only four satellites are tracked. Using the algorithm and real GPS data collected
at a 100-km baseline, this contribution investigates how DGPS positioning accuracies vary with the type of observables used
at reference and mobile stations, and how important it is to choose an elevation-dependent standard deviation for code observations
in DGPS data reduction. It was found that using carrier observations along with code observations is more important at the
reference station than at the mobile station. Choosing an elevation-dependent standard deviation for code observations can
result in better positioning accuracy than choosing a constant standard deviation for code observations. For the 100-km baseline,
half-metre single-epoch positioning accuracy was achieved when dual-frequency data was used at both reference and mobile stations.
The positioning accuracy became better than 0.75m when the types of observable used at the mobile station were replaced by
L1 code and carrier.
Received: 9 April 1996 / Accepted: 6 February 1997 相似文献
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针对常规GNSS解算模糊度存在的问题,该文提出了一种新的GNSS宽巷模糊度单历元求解算法。利用单历元双频码伪距观测值和载波相位观测值得到双差宽巷模糊度浮点解,将所有浮点宽巷模糊度分别向上、向下取整建立模糊度搜索空间;将模糊度空间中的所有备选组合代入双差宽巷观测方程中进行最小二乘解算,其中单位权中误差最小的组合就是最优的宽巷模糊度组合;然后对最优组合进行正确性检验以确定宽巷模糊度。确定宽巷模糊度后,可以利用宽巷观测值和载波观测值求出基础模糊度整周解。实验表明,该文提出的模糊度固定方法具有较高的成功率和可靠性,静态数据中模糊度固定成功率达到98.84%,动态数据中模糊度固定成功率达到了99.60%。 相似文献
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GPS code pseudorange measurements exhibit group delay variations at the transmitting and the receiving antenna. We calibrated C1 and P2 delay variations with respect to dual-frequency carrier phase observations and obtained nadir-dependent corrections for 32 satellites of the GPS constellation in early 2015 as well as elevation-dependent corrections for 13 receiving antenna models. The combined delay variations reach up to 1.0 m (3.3 ns) in the ionosphere-free linear combination for specific pairs of satellite and receiving antennas. Applying these corrections to the code measurements improves code/carrier single-frequency precise point positioning, ambiguity fixing based on the Melbourne–Wübbena linear combination, and determination of ionospheric total electron content. It also affects fractional cycle biases and differential code biases. 相似文献