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1.
利用Hector软件解算我国东北地区16个陆态网络连续站近10 a的时间序列观测数据,获取连续站坐标残差时间序列数据,进而确定最优噪声模型,最终得出基于有色噪声(CN)以及环境负载改正后的速度场. 结果表明:东北地区陆态网络坐标时间序列数据中主要存在白噪声(WN)、闪烁噪声(FN)与幂律噪声(PL);北(N)和天顶(U)方向的最优噪声模型为WN+FN;E方向的最优噪声模型均为WN+PL. 在顾及CN及环境负载的影响下,东北地区陆态网络基于ITRF14框架下在N方向上运动的平均速率为?13.003 mm/a,东(E)方向上运动的平均速率为27.020 mm/a,U方向上运动的平均速率为0.528 mm/a,整体呈隆升趋势. 相似文献
2.
We have used up to 12 years of data to assess DORIS performance for geodynamics applications. We first examine the noise characteristics of the DORIS time-series of weekly station coordinates to derive realistic estimates of velocity uncertainties. We find that a combination of white and flicker noise best explains the DORIS time-series noise characteristics. Second, weekly solutions produced by the Institut Géographique National/Jet Propulsion Laboratory (IGN/JPL) DORIS Analysis Centre are combined to derive a global velocity field. This solution is combined with two independent GPS solutions, including 11 sites on Nubia and 5 on the Somalia plate. The combination indicates that DORIS horizontal velocities have an average accuracy of 3 mm/year, with best-determined sites having velocity accuracy better than 1 mm/year (one-sigma levels). Using our combined velocity field, we derive an updated plate kinematics model with a focus on the Nubia–Somalia area. Including DORIS data improves the precision of the angular velocity vector for Nubia by 15%. Our proposed model provides robust bounds on the maximum opening rates along the East African Rift (4.7–6.7 mm/year). It indicates opening rates 15 and 7% slower than values predicted by NUVEL-1A for the southern Atlantic Ocean and Indian Ocean, respectively. These differences are likely to arise from the fact that NUVEL-1A considered Africa as a single non-deforming plate, while here we use a more refined approach. 相似文献
3.
近年来,有研究发现在GPS测站坐标时间序列中既存在白噪声,也存在有色噪声。为了研究有色噪声对东南极区域GPS测站三维速度估计的影响,本文使用GAMIT/GLOBK10.5软件对东南极区域6个连续GPS测站2005—2014年的实测数据进行解算和平差,并利用最大似然法（MLE）分别估计了在两种假设噪声模型条件下的测站三维运动速度及其不确定性。结果表明：在进行参数估计时,考虑两种有色噪声（闪烁噪声和随机游走噪声）对东南极区域GPS测站三维速度估计的量级影响不大,水平方向最大影响量级为0.3 mm/a,垂直方向最大影响量级为0.8 mm/a;但如果不考虑有色噪声,会严重低估参数估计的真实不确定性。 相似文献
4.
针对北京市CORS站的稳定性问题,该文利用GAMIT/GLOBK软件对北京市13个CORS站2016—2018年的观测数据进行了处理,获取了原始坐标时间序列和坐标残差时间序列,通过极大似然估计的方法对CORS基准站进行了噪声模型分析和区域速度场估计。结果表明,北京市CORS站坐标时间序列的最佳噪声模型为WN+FN+RWN组合模型;采用NEU方向的最佳噪声组合模型对北京市CORS站进行区域速度场估计,BJTZ、CHAO、DSQI、XNJC站的沉降较为严重,其他CORS站N方向速度估值在7.2~14.3 mm/a,E方向速度估值在27.5~32.5 mm/a,U方向速度估值在2.0~8.5 mm/a。 相似文献
5.
噪声分析对GPS时间序列分析有着重要影响,然而针对时间跨度较长的大尺度GPS网的共模误差相关研究较少。本文选取了平均基线长度大于2000 km的欧洲地区9个GPS台站2006-2014年的数据,使用主成分分析法剔除坐标时间序列的共模误差,同时利用极大似然估计的方法对滤波前后的时间序列进行了噪声分析。结果表明,欧洲地区广域GPS网的噪声模型存在多样性,各个分量具有不同的噪声特性,主要表现为白噪声+闪烁噪声、白噪声+幂率噪声,少部分台站N、E两个方向含有随机漫步噪声。经过空间滤波后,部分台站最优噪声模型发生改变,但仍以白噪声+闪烁噪声、白噪声+幂率噪声为主。滤波对N、E方向速度场影响为0.2 mm/a,U方向速度场影响为0.5 mm/a。 相似文献
6.
文中以298个验潮站作为研究对象,采用广义高斯-马尔科夫模型(GGM)、自回归滑动平均模型(ARMA)以及分形自回归聚合滑动平均模型(ARFIMA)三种模型,对验潮站坐标时间序列噪声模型特性及海平面变化趋势进行估计分析,并探讨了时间跨度对验潮站速度估计的影响. 实验结果表明:验潮站坐标时间序列主要呈现为ARFIMA(1,0)、ARFIMA(2,2)、ARMA (1,0) 噪声特性;验潮站速度估计结果表明64.77%的站点速度值所处区间为0～4 mm/a,平均海平面速度为1.25 mm/a,整体处于上升趋势. 随着时间跨度的增加,验潮站坐标序列速度不确定度逐渐由发散趋于收敛,大于110 a的时间跨度有助于获取稳健的验潮站速度估计值. 相似文献
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本文描述了CORS站高程时间序列采用固定周期项建立线性速度场的基本概念，指出给定周期与实际周期存在偏差的问题。为此，提出了CORS站高程时间序列非线性速度场建模方法。该方法以线性最小二乘解作为迭代初值，利用高斯-牛顿迭代算法求解非线性速度场模型的未知参数，实现了CORS站高程时间序列数据的非线性建模；给出了拟合模型残差平方序列异方差特性的检验方法，阐述了建立GARCH（p，q）模型反映CORS站高程非平稳序列波动情况的基本准则。本文以国内外6个CORS站20余年的高程时间序列为研究对象，建立非线性速度场运动模型。结果表明：CORS站高程运动并不存在严格的整年或半年周期项，近似年周期运动最为明显，近似两年周期运动占比最小，年周期估计偏差达到12%，半年周期偏差18%，两年周期偏差6%，非线性建模精度和效果整体优于线性模型。利用ARCH检验法得到CORS站高程非线性模型的残差平方序列存在异方差性，即残差平方序列具有非平稳特性，引入GARCH（p，q）模型对CORS站高程分量非平稳残差平方序列建模，反映了残差平方序列的非平稳波动。验证了GARCH（p，q）模型对CORS站高程非平稳残差平方序列建模的可行性，为今后利用GARCH（p，q）模型对CORS站高程非平稳噪声序列建模和非线性速度场重构提供了思路。 相似文献
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In the frame of the International DORIS Service (IDS), the Laboratoire d’Etudes en Géophysique et Océanographie Spatiales (LEGOS)/Collecte Localisation Satellites (CLS) Analysis Center (LCA) processes DORIS measurements from the SPOT, TOPEX/Poseidon and Envisat satellites and provides weekly station coordinates of the whole network to the IDS. Based on DORIS measurements, the horizontal and vertical velocities of 57 DORIS sites are computed. The 3D positions and velocities of the stations with linear motion are estimated simultaneously from the 12-year (1993–2004) combined normal equation matrix. We include 35 DORIS sites assumed to be located in the stable zones of 9 tectonic plates. For the motion of these plates, we propose a model (LCAVEL-1) of angular velocities in the ITRF2000 reference frame. Based on external comparison with the most recent global plate models (PB2002, REVEL, GSRM-1 and APKIM2000) and on internal analysis, we estimate an average velocity error of the DORIS solution of less than 3 mm/year. The LCAVEL-1 model presents new insights of the Somalia/Nubia pair of plates, as the DORIS technique has the advantage of having a few stations located on those two plates. We also computed (and provide in this article) the horizontal motion of the sites located close to plate boundaries or in the deformation zones defined in contemporary models. These computations could be used in further analysis for these particular regions of the Earth not moving as rigid plates. 相似文献
10.
获取准确的GNSS测站速度对于研究全球板块运动、地壳形变、地震活动及其地球动力学过程至关重要。为此,以GNSS基线解算后的基线向量作为观测值,重建了最小二乘综合速度解算模型和卡尔曼滤波速度估计模型。模型中,考虑了测站坐标、运动速度、年、半年周期项一同作为参数,在基线解网平差的同时,一并求解获取速度估值。同时,利用坐标时序分析的方法,顾及白噪声和幂律噪声的影响,对单日解坐标时间序列重建了时序速度拟合估计模型,以获取长期趋势项作为速度值。基于3种模型,对川滇地区中国地壳运动观测网络2010—2014年21个GPS基准站的观测数据进行了速度估计与对比分析。结果表明:3种模型所估计测站速度非常接近,差异基本处于0~1mm/a范围之内;速度估值中误差均在亚毫米水平。由此得出,3种速度估计模型具有本质的一致性,均可正确估计测站运动速度,能够满足高精度地壳形变研究的需要。 相似文献
11.
Fast error analysis of continuous GPS observations 总被引：4，自引：1，他引：3
It has been generally accepted that the noise in continuous GPS observations can be well described by a power-law plus white
noise model. Using maximum likelihood estimation (MLE) the numerical values of the noise model can be estimated. Current methods
require calculating the data covariance matrix and inverting it, which is a significant computational burden. Analysing 10 years
of daily GPS solutions of a single station can take around 2 h on a regular computer such as a PC with an AMD AthlonTM 64 X2 dual core processor. When one analyses large networks with hundreds of stations or when one analyses hourly instead
of daily solutions, the long computation times becomes a problem. In case the signal only contains power-law noise, the MLE
computations can be simplified to a process where N is the number of observations. For the general case of power-law plus white noise, we present a modification of the MLE equations
that allows us to reduce the number of computations within the algorithm from a cubic to a quadratic function of the number
of observations when there are no data gaps. For time-series of three and eight years, this means in practise a reduction
factor of around 35 and 84 in computation time without loss of accuracy. In addition, this modification removes the implicit
assumption that there is no environment noise before the first observation. Finally, we present an analytical expression for
the uncertainty of the estimated trend if the data only contains power-law noise.
Electronic supplementary material The online version of this article (doi: ) contains supplementary material, which is available to authorized users. 相似文献
12.
为了评估北斗卫星导航系统（BeiDou navigation satellite system, BDS）监测中国大陆地区地壳变形的技术能力,利用GAMIT/GLOBK软件处理了2017—2019年中国大陆构造环境监测网络23个基准站的全球定位系统（global positioning system, GPS）与BDS-2双模观测数据。结果显示,北斗二代的水平和垂向单日测站定位精度分别约为5~7 mm和13 mm,基线相对定位精度水平分量达到3~4 mm+（1~2）×10-8,水平位移速度测定精度约为0.6 mm/a。北斗二代的精密定位水平大致与20世纪90年代初GPS相当,可用于测定大尺度的板块运动及板内变形,但受卫星星座和定轨精度限制,不能准确反映季节性变动状态。作为对现有GPS监测的补充,可将基准站3年尺度的地壳运动监测精度最多提高20%。 相似文献
13.
选取ITRF2008框架下格陵兰岛区域12个GPS站2013年1月-2016年12月期间的日解坐标时间序列作为研究对象，并利用极大似然估计分析地表质量负载改正前后各站点的噪声特性、速度场及周期项振幅。结果表明：站点最优噪声模型主要为白噪声+幂律噪声与白噪声+闪烁噪声，地表质量负载形变修正GPS坐标时序后，明显增加U方向闪烁噪声的成分，平均降低其速度约0.36 mm/a，对水平方向影响较小；同时分别降低高程方向44.1%、14.2%的1 a项、0.5 a项振幅，相反，却增加了水平方向的周期项振幅。 相似文献
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利用小波谱分析了中国区域IGS（International GNSS Service）站坐标时间序列中周期信号成分及其随时间的变化,根据小波谱中小波系数的能量在时域上的变化对时间序列进行分段,然后采用方差-协方差验后估计法分析了白噪声+闪烁噪声组合模型下测站在不同时间段的运动特征及变化规律。结果表明,中国区域的IGS站运动特征在不同时间段内是变化的,其中URUM站垂直速度变化大于4 mm,BJFS以及CHAN站水平速度变化大于2 mm,其余站速度变化均在2 mm以内;周年、半周年信号的振幅也均有差异,其中BJFS站垂直分量周年振幅变化最大,超过5 mm;此外,强度较弱的其他周期项存在于分段时间序列中,但其对速度、周期振幅以及噪声分量估计结果影响较小;对时间序列进行分段估计,所得的参数不同,其相差程度可反映出不同时间段内的板块运动等地球物理因素变化的差异。 相似文献
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利用中国地震局全球卫星导航系统(GNSS)数据产品服务平台获取内蒙古自治区境内15个陆态网络连续站2010-06—2021-06的观测数据,通过GAMIT/GLOBK软件、HECTOR软件解算得到去奇异值后的坐标时间序列,最后结合贝叶斯信息量准则(BIC)数值分析确定最优噪声模型:内蒙古自治区坐标时间序列在东(E)方向的最优模型为白噪声+闪烁噪声 (WN+FN),在北(N)和天顶(U)方向的最优噪声模型为白噪声+幂律噪声(WN+PL). 采用最佳噪声模型对速度场进行修正,在ITRF14框架下,内蒙古地区陆态网络连续站的平均运动速率为30.653 mm/a,运动方向为26°57′51″SEE;垂直方向上平均运动速率为0.792 mm/a. 相似文献
16.
K. Le Bail 《Journal of Geodesy》2006,80(8-11):541-565
The noise spectrum in DORIS ground- station motion is investigated by means of the Allan variance method applied to the decomposition of the 3D signal into its principal components in the time domain. Sets of weekly position time-series from 1994 to 2005 derived by three IDS Analysis Centres (IGN-JPL, INASAN, and LEGOS-CLS) for 119 stations at 69 sites are considered. The observing satellites are SPOT-2, SPOT-3, SPOT-4, and SPOT-5, TOPEX/Poseidon, and ENVISAT. Annual and semi-annual perturbations, as well as the 117.3-day term associated with the TOPEX/Poseidon orbit, are found at most stations. Their amplitudes reach up to 19.3, 23.7, and 13.3 mm, respectively, for the three analysis centres (ACs). When corrected for these components and a linear drift, the time-series dominantly show white noise (WN) at the 10–45mm level the noise level is the highest in the East direction, probably in connection with the high orbit inclinations. The noise level is minimum for the high latitude stations, mostly and intensively observed by the SPOT satellites, and the determination of the noise type is unclear; longer observation spans would be needed to decide between interannual variations and flicker noise. The improvement in positioning due to the DORIS constellation extension from three to five satellites in 2002, and the network rejuvenation program initiated in 2000, results in a decrease of the noise level by a factor of 1.7 in a WN context, both before and after the changes. One example of the benefit of studying the signal in the time eigenspace domain is the detection of anomalously large WN in the East direction for station HBKB (Hartebeesthoek, Africa) that masks the above-mentioned improvement. Studying the projection on the local frame of the second and third time-eigenspace components, a noise excess is detected in the North direction for some of the ACs. Station stability derived from our time-series analysis confirms, in general, the expected performance based on the careful technical review of the station components (antenna, pillar, etc.). The respective merits of our noise qualification method, based on direct time-series analysis in the time-eigenspace domain without any a priori statistical model, in comparison with other methods, such as the selection of a mixed-noise model by maximum likelihood estimation, are discussed. 相似文献
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18.
Zinovy Malkin 《Journal of Geodesy》2013,87(6):505-514
UT1 estimates obtained from the very long baseline interferometry (VLBI) Intensives data depend on the station displacement model used during processing. In particular, because of seasonal variations, the instantaneous station position during the specific intensive session differs from the position predicted by the linear model generally used. This can cause systematic errors in UT1 Intensives results. In this paper, we first investigated the seasonal signal in the station displacements for the 5 VLBI antennas participating in UT1 Intensives observing programs, along with the 8 collocated GPS stations. It was found that a significant annual term is present in the time series for most stations, and its amplitude can reach 8 mm in the height component, and 2 mm in horizontal components. However, the annual signals found in the displacements of the collocated VLBI and GPS stations at some sites differ substantially in amplitude and phase. The semiannual harmonics are relatively small and unstable, and for most stations no prevailing signal was found in the corresponding frequency band. Then two UT1 Intensives series were computed with and without including the seasonal term found in the previous step in the station movement model. Comparison of these series has shown that neglecting the seasonal station position variations can cause a systematic error in UT1 estimates, which can exceed 1 $\upmu $ s, depending on the observing program. 相似文献
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20.
Multi-technique comparison of tropospheric zenith delays derived during the CONT02 campaign 总被引：2，自引：7，他引：2
In October 2002, 15 continuous days of Very Long Baseline Interferometry (VLBI) data were observed in the Continuous VLBI 2002 (CONT02) campaign. All eight radio telescopes involved in CONT02 were co-located with at least one other space-geodetic technique, and three of them also with a Water Vapor Radiometer (WVR). The goal of this paper is to compare the tropospheric zenith delays observed during CONT02 by VLBI, Global Positioning System (GPS), Doppler Orbitography Radiopositioning Integrated by Satellite (DORIS) and WVR and to compare them also with operational pressure level data from the European Centre for Medium-Range Weather Forecasts (ECMWF). We show that the tropospheric zenith delays from VLBI and GPS are in good agreement at the 3–7 mm level. However, while only small biases can be found for most of the stations, at Kokee Park (Hawaii, USA) and Westford (Massachusetts, USA) the zenith delays derived by GPS are larger by more than 5 mm than those from VLBI. At three of the four DORIS stations, there is also a fairly good agreement with GPS and VLBI (about 10 mm), but at Kokee Park the agreement is only at about 30 mm standard deviation, probably due to the much older installation and type of DORIS equipment. This comparison also allows testing of different DORIS analysis strategies with respect to their real impact on the precision of the derived tropospheric parameters. Ground truth information about the zenith delays can also be obtained from the ECMWF numerical weather model and at three sites using WVR measurements, allowing for comparisons with results from the space-geodetic techniques. While there is a good agreement (with some problems mentioned above about DORIS) among the space-geodetic techniques, the comparison with WVR and ECMWF is at a lower accuracy level. The complete CONT02 data set is sufficient to derive a good estimate of the actual precision and accuracy of each geodetic technique for applications in meteorology. 相似文献