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针对现有GPS数据处理过程中多余长基线对高精度GPS数据解算影响方面研究较少,文中选择具有不同已知点分布的两种CORS网观测数据,并按照解算时间分为4 h、6 h、8 h、12 h、18 h和24 h共6个时段,以定量分析在不同已知点分布和解算时间时多余长基线对高精度GPS数据解算的影响。最终得出,多余长基线的存在会对GPS数据解算的精度产生影响,且随着解算时间的增加,其影响呈减小趋势;多余长基线的存在也会对解算结果产生较大影响,在已知点分布较差时,影响最大值达到了12.7 mm,在已知点分布较好时最大值也达到了6 mm,且在各时段内,影响均较为明显。因此在进行高精度GPS数据解算时,需考虑多余长基线的影响。 相似文献
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探讨了中长基线GPS观测值随机特性的评估方法,先采用历元间高次差分的高通滤波算法有效地消除低频系统误差,只保留高频噪声;然后建立评估中长基线观测值精度、交叉相关性和时间相关性的数学模型。实测数据计算分析了GPS观测值的精度与高度角的关系、不同类型观测值的交叉相关性以及各类观测值的时间相关性。 相似文献
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首先从参数估计、精度评定和质量控制角度论证了在精密定位中随机模型的重要性;然后基于短基线单差观测模型,采用严密的方差分量估计方法计算了不同频率、不同卫星的相位和伪距观测值精度,任意频率之间的交叉相关性以及不同频率的相位和伪距观测值在不同时间间隔上的时间相关性;随后分析了随机模型对基线精度和整体检验统计量的影响。结果表明：北斗用户接收机数据精度都与高度角相关,建议采用高度角指数加权函数;北斗二号3个频率相位观测值之间存在不同程度的相关性,其他类型观测值之间的交叉相关性不明显,不同频率的相位和伪距观测值时间相关性较明显,高精度应用中需关注。另外,正确的随机模型计算的基线精度更接近理论精度。本文为用户正确认识北斗系统3个类型卫星观测信息、正确使用北斗系统提供支撑。 相似文献
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现代大地测量数据中往往存在时间相关性,忽略观测值时间相关性会影响参数估值的精度和可靠性。因此,本文研究了几种时间相关观测的动态数据处理方法。首先,对观测值时间相关性的处理方法进行了扩展和统一。利用极大验后估计原理,提出了第3种思路,并在无历元公用参数和有历元公用参数两类模型下,详细推导了去相关变换法、差分变换法和极大验后估计法这3种思路的动态解,并对它们的特点和等价性进行了论证。其次,为了平衡实际应用中的解算效率且同时有效顾及时间相关性,利用自相关函数表达时间相关性,导出了相应退化形式。最后,通过GPS实测数据验证了本文理论公式的正确性和实用性。 相似文献
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《测绘地理信息》2017,(2)
研究BDS/GPS在鄂北水资源配置工程宝林隧道控制网中的应用,利用宝林隧道二等GNSS控制网2016年4个观测时段数据,分别采用BDS、GPS、BDS+GPS三种模式解算各个时段的基线向量,并以GAMIT的解算值作参考进行成果的精度分析。基线向量结果表明,BDS可以满足宝林隧道的测量精度要求,但在观测条件不佳时,需对观测数据进行筛选,去除噪声较大的历元观测值。对比BDS、GPS单系统基线结果,N与E方向差异可以保持在5mm左右,U方向大部分保持在10mm左右,BDS+GPS观测数据解算精度高于任何一种单系统。不同数据的平差结果精度指标均符合规范。同时对点位进行稳定性分析,不同数据分析结果基本一致。 相似文献
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讨论了隧道洞内外贯通误差的计算方法,利用国内外对GPS观测值时间相关性的研究,得到不顾及时间相关性的基线验后精度与实际精度的比例因子,并应用于隧道洞外GPS控制网贯通误差的计算,使该值更为真实、可靠,从而更好的确定后续测量等级与方案。 相似文献
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基于北斗卫星的几何观测模型,处理3种型号接收机的4组短基线和零长度基线北斗观测数据,通过与MINQUE方法估计的随机模型进行比较,验证直接利用残差估值计算北斗观测值随机模型的可行性;在此基础上分析北斗卫星观测值高度角相关的精度、交叉相关性、空间相关性和时间相关性;结果表明北斗对地静止轨道(GEO)卫星的观测误差、空间相关性、时间相关性均大于倾斜同步轨道(IGSO)卫星和中轨道(MEO)卫星;北斗卫星的同类型观测值之间均具有较强的交叉相关性,不同类型观测值间的交叉相关性较弱,且随机模型的估计结果受接收机的内部误差和测站的外部误差影响. 相似文献
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星载重轨干涉SAR卫星在高程测绘和形变测量中有着全天时全天候和大范围的优势,其中干涉基线是决定干涉性能的重要指标,而卫星重访轨道对干涉基线起着决定性的作用。通过对现有高分三号干涉数据轨道参数的分析,发现干涉基线相比国外先进卫星过长且稳定性有待提高。本文通过对相对轨道根数和机动控制的分析,得到满足重轨干涉SAR系统要求的稳定基线。以第一次观测的轨道为参考轨道,基于在摄动情况下重复观测轨道与参考轨道的相对轨道根数,计算得到重轨干涉基线的变化规律,并对不同纬度的观测目标进行了样例分析。在基线变化规律的基础上,利用机动速度和相对轨道根数的关系,进一步计算得到满足基线状态需求的机动控制方法。通过实际数据分析,给出了相对轨道根数变化对初始理想构型的影响,验证了重轨干涉基线变化规律符合本文的分析,并利用仿真样例给出了使得重轨干涉基线达到预期要求的机动控制方案。实际数据和仿真实验表明该模型能够通过可长时间观测并准确获得的轨道根数直接计算基线状态,并能从干涉基线需求出发,快速准确的得出对卫星的控制策略。 相似文献
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Performance analysis of triple-frequency ambiguity resolution with BeiDou observations 总被引：5，自引：1，他引：4
We investigate triple-frequency ambiguity resolution performance using real BeiDou data. We test four ambiguity resolution (AR) methods which are applicable to triple-frequency observations. These are least squares ambiguity decorrelation adjustment (LAMBDA), GF-TCAR (geometry-free three-carrier ambiguity resolution), GB-TCAR (geometry-based three-carrier ambiguity resolution) and GIF-TCAR (three-carrier ambiguity resolution based on the geometry-free and ionospheric-free combination). A comparison between LAMBDA, GF-TCAR and GB-TCAR was conducted over three short baselines and two medium baselines. The results indicated that LAMBDA is optimal in both short baseline and medium baseline cases. However, the performances of GB-TCAR and LAMBDA differ slightly for short baselines. Compared with GF-TCAR, which uses the geometry-free model, the GB-TCAR using the geometry-based model improves the AR performance significantly. Compared with dual-frequency observations, the LAMBDA AR results show a significant improvement when using triple-frequency observations over short baselines. The performance of GIF-TCAR is evaluated using multi-epoch observations. The results indicated that multi-path errors on carrier phases will have a significant influence on GIF-TCAR AR results, which leads to different GIF-TCAR AR performance for different type of satellites. For GEO (Geostationary Orbit) satellites, the ambiguities can barely be correctly fixed because the multi-path errors on carrier phases are very systematic. For IGSO (Inclined Geosynchronous Orbit) and MEO (Medium Earth Orbit) satellites, when the elevation cutoff angle is set as 30°, several tens to several hundreds of epochs are needed for correctly fixing the narrow lane ambiguities. The comparison of positioning performance between dual-frequency observations and triple-frequency observations was also conducted. The results indicated that a minor improvement can be achieved by using triple-frequency observations compared with using dual-frequency observations. 相似文献
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国家高精度GPS网整体平差中的粗差分析 总被引：1，自引：0，他引：1
分析了国家高精度ＧＰＳ网中的粗差观测量的特点,提出了采用相关分析的粗差探测理论,对国家高精度ＧＰＳ网的各子网和相邻子网进行粗差探测,并采用稳健估计的平差方法,消除粗差对平差结果的影响,大大提高了国家高精度ＧＰＳ网的整体平差精度。 相似文献
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本文根据地-月相对运动特征,建立了月基重轨InSAR观测几何模型,使用NASA/JPL高精度DE430月球星历数据,计算了月基SAR的重访时间以及对应的空间基线。结果表明:月基SAR的重返周期约24.8h;由于月球南北向速度发生周期性变化,月基重轨InSAR垂直基线长度会随重访次数产生较大变化,且基线长度近似呈现1恒星月周期变化特征。在空间基线约束下,本文进一步分析了月基重轨InSAR时-空基线特征,研究发现:①在确定的初始观测条件下,只能在特定的时间基线上实现月基重轨InSAR观测,并且初始观测时间不同,可实现月基重轨InSAR观测的时间基线也不同;②不同的时间基线可形成干涉组合个数不同,约50%的干涉组合个数对应的时间基线接近1恒星月及其整数倍;不同的观测位置可形成干涉组合个数不同,约80%的干涉组合个数发生在月球赤纬大于10°区域。因此,月基重轨InSAR观测数据获取计划的设计应综合考虑时间基线、空间基线以及初始观测时间等因素。 相似文献
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Kees De Jong 《GPS Solutions》1999,3(2):11-18
In this article, the influence of biases in GPS code observations on the estimated parameters of the geometry-free model is
investigated. This is done for undifferenced as well as double-differenced data from short baselines, that is, baselines for
which ionospheric effects may be assumed absent. It is shown how introducing a linear model for code multipath affects the
original model parameters. The performance of the original and extended model is illustrated by analyzing data from a single
receiver and a short baseline. ? 1999 John Wiley & Sons, Inc. 相似文献
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Most stochastic modelling techniques neglect the correlations among the raw un-differenced observations when forming the variance–covariance matrix of the Global Navigation Satellite System (GNSS) observations. Some methods were developed to model these correlations. One such method is the Minimum Norm Quadratic Unbiased Estimator (MINQUE). Studies have shown that MINQUE improves ambiguity resolution, and ultimately, the positioning solution in short baselines. However, its effect in cases of processing with longer baselines and on the estimation of zenith wet delay (ZWD) is somewhat unknown. In this paper, a comparison between the impact of neglecting the correlations among the observations using an elevation-angle-dependent model (EADM) and modelling the correlations using MINQUE on height determination and ZWD for medium and long baselines is carried out. The initial testing was carried out across two Australian GNSS stations with a medium-length baseline throughout a three-week campaign. The results showed that using MINQUE did not resolve the coordinate, height and wet delay components as accurately as the EADM. The results were further verified with two long-baseline campaigns whereby EADM was also able to provide better wet delay estimates. The coordinate results were, however, mixed. Overall, the study concluded that the inclusion of the correlations among the observations, in general, do not improve the resolution of the coordinate and wet delay estimates. 相似文献
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利用GPS载波相位观测值进行基线测定具有重要意义。本文讨论了基线测定中卫星星历误差对定位结果的影响,提出了基线上轨道改进的定位方法,编制了基线测定的定位软件,并使用高精度基线上的实际观测资料进行了计算。计算结果表明在基线上用轨道改进定位方法是可行的,可以提高定位精度。 相似文献
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在PSInSAR干涉测量技术中,主影像的选择直接影响后续的形变相位提取及沉降信息解算。在综合考虑空间垂直基线、时间基线和多普勒中心频率对影像去相干影响的基础上,将三因素的相干性测度映射到三维空间,构成三个质点,通过对三质点的质心的研究来衡量三因素对影像相干性的综合影响,构建一种新的主影像选择模型。以2003~2009年北京地区28景ENVISAT ASAR影像为试验数据,分别采用该模型及综合最大相关系数模型进行主影像选择,并进行实际干涉处理,以生成干涉图及相干系数均值,对两种方法主影像选取结果进行定量评价。结果表明,与直接以去相干因素的相干测度乘积构建的综合相关系数模型相比,该方法选取的主影像更为合理,与其他辅影像总体干涉性更好。 相似文献
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为分析北斗卫星观测值随机特性,估计了地球静止轨道、倾斜地球同步卫星轨道、中地球轨道卫星载波相位观测值的方差分量。发现不同接收机和不同类型卫星观测值方差分量的大小和时变特性具有明显差异。为构建更切实际的方差结构随机模型,提出利用迭代最小二乘和最小范数二次无偏估计相结合的方法,实时估计不同类型北斗卫星观测值方差分量。为评估实时估计随机模型的性能,对243 m、645 m、10 137 m三条不同长度基线进行精密相对定位测试,结果表明:实时估计随机模型能有效改善北斗卫星精密单历元动态相对定位性能,尤其当站间距离较长时改善更显著。10 137m基线测试结果表明,1h数据单历元解在北、东、高方向,平均定位精度分别提高了41.3%、54.5%、51.6%,稳定性分别提高了38.4%、17.7%、39.7%。 相似文献
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As a first step towards studying the ionosphere with the global navigation satellite system (GNSS), leveling the phase to the code geometry-free observations on an arc-by-arc basis yields the ionospheric observables, interpreted as a combination of slant total electron content along with satellite and receiver differential code biases (DCB). The leveling errors in the ionospheric observables may arise during this procedure, which, according to previous studies by other researchers, are due to the combined effects of the code multipath and the intra-day variability in the receiver DCB. In this paper we further identify the short-term temporal variations of receiver differential phase biases (DPB) as another possible cause of leveling errors. Our investigation starts by the development of a method to epoch-wise estimate between-receiver DPB (BR-DPB) employing (inter-receiver) single-differenced, phase-only GNSS observations collected from a pair of receivers creating a zero or short baseline. The key issue for this method is to get rid of the possible discontinuities in the epoch-wise BR-DPB estimates, occurring when satellite assigned as pivot changes. Our numerical tests, carried out using Global Positioning System (GPS, US GNSS) and BeiDou Navigation Satellite System (BDS, Chinese GNSS) observations sampled every 30 s by a dedicatedly selected set of zero and short baselines, suggest two major findings. First, epoch-wise BR-DPB estimates can exhibit remarkable variability over a rather short period of time (e.g. 6 cm over 3 h), thus significant from a statistical point of view. Second, a dominant factor driving this variability is the changes of ambient temperature, instead of the un-modelled phase multipath. 相似文献