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1.
处理了2008-01~2009-03的VLBI观测数据,提取了日长变化信息,并与IVS网站的结果进行了对比;计算了日长变化的月周期长度和半月周期长度;利用近几年VLBI数据中的日长变化信息绘制日长变化曲线,分析了日长的季节性变化及引起日长变化的因素。  相似文献   

2.
目前正处在下一代甚长基线干涉测量(very long baseline interferometry,VLBI)系统的建设时期。利用维也纳VLBI与卫星软件(Vienna VLBI and satellite software,VieVS)解算了2006—2015年的VLBI数据,得到了10 a的地球定向参数(Earth orientation parameters,EOP)时间序列,并与国际地球自转服务机构的结果进行了对比。利用解算结果得到了10 a的日长变化时间序列,通过傅里叶分析得出了日长变化的短周期、半月周期、月周期、半年周期和周年周期,同时还分析得到了极移序列中的周年项和张德勒周期项以及章动改正序列中的自由核章动项。此次解算工作可为武汉大学卫星台站日后的VLBI数据解析积累一定的经验。  相似文献   

3.
针对传统的对流层天顶延迟模型在估算天顶延迟中存在精度不高和稳定性差的问题,提出了一种在Hopfield模型基础上增加年周期和半年周期项的方法。该方法利用中国区域45个站2012—2014年的全球大地测量观测系统大气数据,分析了天顶对流层延迟以及Hopfield模型残差的时间序列和频谱分布规律,由此引入年周期和半年周期项,建立了适应中国区域的GHop模型,并对两种模型在中国区域的精度和适应情况进行了评估。结果表明:Hopfield模型的偏差和均方根在时间上呈现明显的季节变化特征,而GHop模型的偏差和均方根变化较小且稳定;在空间分布上,Hopfield模型随着高程和纬度增加,偏差和均方根变化幅度大,而GHop模型能够适应不同纬度和高程的变化范围;GHop模型的内符合精度较Hopfield模型提高28%,使用中国区域76个无线电探空数据进行外符合检验,统计结果同样优于Hopfield模型。所提方法计算的天顶对流层延迟结果更加可靠,具备较高的实用价值。  相似文献   

4.
为了探索地表质量迁移对日长变化的激发作用,文章在原始日长变化中扣除了固体潮、10年尺度信号、风和洋流效应,得到残余日长变化.然后分别利用AOH气候模型、SLR数据和CSR、GFZ、JPL提供的RL05版本的GRACE月重力场模型,计算了地表质量迁移对日长变化的激发作用.通过分析发现,和SLR、AOH质量激发相比,在季节性尺度上,3种GRACE质量激发能够更好地解释残余日长变化中周年和半周年的起伏,尤其是在周年项上,3种GRACE质量激发和残余日长变化间十分接近;在季节内尺度上,GRACE (GFZ)质量激发同样可以更好地解释残余日长变化,而GRACE(GFZ)和GRACE(JPL)质量激发由于包含一个周期为5.6个月的信号,与残余日长变化的相干性很低.  相似文献   

5.
处理了2000-01~2012-06的VLBI观测数据,提取了ERP地球自转参数信息,通过JPL的DE405星历计算得到了2000-01~2012-06的月地距时间序列;消除日长变化、极移和月地距时间序列趋势项,采用频谱分析的方法求得它们的周期;根据解算的周期推测日长变化和日地距可能存在相关性,并验证了推测.  相似文献   

6.
日长季节振荡的振幅变化与南方涛动现象   总被引:2,自引:0,他引:2  
闫昊明  钟敏  朱耀仲 《测绘学报》2000,29(Z1):103-106
本文提出了小波振幅谱的定义,给出了其在频域的表达式及频域周期与Fourier周期之间的线性关系。通过与谐波分析比较,证明了小波振幅谱应用的有效性。应用小波振幅谱研究了日长季节振幅变化与南方涛动之间的关系,结果表明日长周年振荡的振幅变化与南方涛动的年际变化呈明显负相关,而日长半年振荡的振幅变化与其呈更强的正相关。  相似文献   

7.
地心运动时间序列的抗差谱分析   总被引:6,自引:1,他引:6  
本文将抗差估计与谱分析相结合,提出了抗差谱分析。用该方法对全球约120个IGS站5年GPS观测结果求得的地心运动时间序列进行了分析,发现地心运动在各方向有不同的主周期变化。X方向受地球物理交叉影响较大,无法分离出对该方向影响较大的主周期变化;而Y,Z方向都有明显的主周期变化。Y方向有明显的年周期变化、半年周期变化、季节性变化和月周期变化,其中,年周期变化的贡献最大;Z方向的主周期是年周期变化、半年周期变化、51天和609天的周期变化。与X,Y方向相比,Z方向振幅明显偏大。  相似文献   

8.
介绍了小波振幅分析方法和小波振周谱分析方法的解析表达,然后利用小波振幅分析方法研究了1950~2003年日长近120d准周期振荡的时频规律(国际地球自转中心提供的1962~2003年的日长变化以及根据美国环境预测中心提供的大气角动量换算的1950~2003年大气激发的日长变化)。此外,还利用小波振周谱分析方法研究了同一时段内厄尔尼诺3、4区海水温度异常年际变化的时频特征,并将它与日长近120d准周期振荡的振幅变化进行了比较。  相似文献   

9.
利用TOPEX/Poseidon(T/P)卫星10年(1992~2002)监测博斯腾湖水位变化的GDR数据,经过数据的地球物理改正、编辑、约化和滤波后,分别采用小波分析和傅里叶分析得到了博斯腾湖水位变化的平均周期为1034d,363d,182d和47d。季节性变化是湖泊水位变化的主项,利用最小二乘法得到了周年振幅为0.7196m,半年振幅为0.5322m,因此季节性变化的主周期是周年,次周期是半年。博斯腾湖水位变化变化趋势为0.2012m/a,说明在全球气候变暖趋势下,博斯腾湖水位在升高。由博斯腾湖月水位变化的时间序列与NINO3 SST进行相关性分析,发现在NINO3 SST 发生6个月后,博斯腾湖月水位变化序列与NINO3 SST数据相关性最大(-0.2784),表明厄尔尼诺事件对我国西部气候影响的具有一定的滞后性。  相似文献   

10.
使用一维连续小波变换方法,分析了1880~2011年全球海洋表面温度平均异常时间序列的变化特征;探讨了全球以及半球在不同时间尺度上的变化、突变点以及一致性;清晰地获得了海温在不同时间层次上的分布和冷暖交替情况。另外,在大尺度上全球海洋表面温度有80 a和40 a附近的2个年代际周期,在中尺度上存在一个12 a和一个19 a的周期,在小尺度上存在一个4~6 a的主周期。  相似文献   

11.
Continuous (CONT) VLBI campaigns have been carried out about every 3 years since 2002. The basic idea of these campaigns is to acquire state-of-the-art VLBI data over a continuous time period of about 2 weeks to demonstrate the highest accuracy of which the current VLBI system is capable. In addition, these campaigns support scientific studies such as investigations of high-resolution Earth rotation, reference frame stability, and daily to sub-daily site motions. The size of the CONT networks and the observing data rate have increased steadily since 1994. Performance of these networks based on reference frame scale precision and polar motion/LOD comparison with global navigation satellite system (GNSS) earth orientation parameters (EOP) has been substantially better than the weekly operational R1 and R4 series. The precisions of CONT EOP and scale have improved by more than a factor of two since 2002. Polar motion precision based on the WRMS difference between VLBI and GNSS for the most recent CONT campaigns is at the 30 \(\upmu \)as level, which is comparable to that of GNSS. The CONT campaigns are a natural precursor to the planned future VLBI observing networks, which are expected to observe continuously. We compare the performance of the most recent CONT campaigns in 2011 and 2014 with the expected performance of the future VLBI global observing system network using simulations. These simulations indicate that the expected future precision of scale and EOP will be at least 3 times better than the current CONT precision.  相似文献   

12.
The very long baseline interferometry (VLBI) Intensive sessions are typically 1-h and single-baseline VLBI sessions, specifically designed to yield low-latency estimates of UT1-UTC. In this work, we investigate what accuracy is obtained from these sessions and how it can be improved. In particular, we study the modeling of the troposphere in the data analysis. The impact of including external information on the zenith wet delays (ZWD) and tropospheric gradients from GPS or numerical weather prediction models is studied. Additionally, we test estimating tropospheric gradients in the data analysis, which is normally not done. To evaluate the results, we compared the UT1-UTC values from the Intensives to those from simultaneous 24-h VLBI session. Furthermore, we calculated length of day (LOD) estimates using the UT1-UTC values from consecutive Intensives and compared these to the LOD estimated by GPS. We find that there is not much benefit in using external ZWD; however, including external information on the gradients improves the agreement with the reference data. If gradients are estimated in the data analysis, and appropriate constraints are applied, the WRMS difference w.r.t. UT1-UTC from 24-h sessions is reduced by 5% and the WRMS difference w.r.t. the LOD from GPS by up to 12%. The best agreement between Intensives and the reference time series is obtained when using both external gradients from GPS and additionally estimating gradients in the data analysis.  相似文献   

13.
ERP精度对“嫦娥一号”差分VLBI定位精度的影响   总被引:2,自引:0,他引:2  
推导了差分VLBI(ΔDOR)用于月球探测器定位的数学模型,利用嫦娥一号实测数据对探测器的位置和地球自转参数(ERP)同时进行了解算,并分析了ERP先验精度对定位精度的影响。  相似文献   

14.
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   

15.
差分VLBI测量的一种实现方案   总被引:1,自引:0,他引:1  
差分VLBI通过交替观测目标天体和参考天体,将共同的误差因素从观测量中扣除,能够实现高精度的相对定位,因而在深空探测中有重要作用.然而,差分VLBI高精度的实现要求目标天体和参考天体的角距很近,这大大限制了其应用.讨论设计了差分VLBI测量的一种实现方案,利用多颗参考源的观测内插出目标源的非几何时延修正,放宽了对目标源和参考源的角距限制.该方案在S波段对目标源非几何时延的修正精度可以达到1 ns水平.  相似文献   

16.
我国第一台流动甚长基线干涉测量(VLBI)设备经近十年的研制目前在昆明进行了试观测,本文介绍了实验观测及数据的获取情况。并对数据文件进行了处理。结果显示,在上海佘山25米天线至昆明流动站近2千公里的基线上,昆明流动站坐标精度优于5cm。基线相对精度优于10^-8。  相似文献   

17.
差分VLBI通过交替观测目标天体和参考天体,将共同的误差因素从观测量中扣除,能够实现高精度的相对定位,因而在深空探测中有重要作用。然而,差分VLBI高精度的实现要求目标天体和参考天体的角距很近,这大大限制了其应用。讨论设计了差分VLBI测量的一种实现方案,利用多颗参考源的观测内插出目标源的非几何时延修正,放宽了对目标源和参考源的角距限制。该方案在S波段对目标源非几何时延的修正精度可以达到1 ns水平。  相似文献   

18.
The CONT02 campaign is of great interest for studies combining very long baseline interferometry (VLBI) with other space-geodetic techniques, because of the continuously available VLBI observations over 2 weeks in October 2002 from a homogeneous network. Especially, the combination with the Global Positioning System (GPS) offers a broad spectrum of common parameters. We combined station coordinates, Earth orientation parameters (EOPs) and troposphere parameters consistently in one solution using technique- specific datum-free normal equation systems. In this paper, we focus on the analyses concerning the EOPs, whereas the comparison and combination of the troposphere parameters and station coordinates are covered in a companion paper in Journal of Geodesy. In order to demonstrate the potential of the VLBI and GPS space-geodetic techniques, we chose a sub-daily resolution for polar motion (PM) and universal time (UT). A consequence of this solution set-up is the presence of a one-to-one correlation between the nutation angles and a retrograde diurnal signal in PM. The Bernese GPS Software used for the combination provides a constraining approach to handle this singularity. Simulation studies involving both nutation offsets and rates helped to get a deeper understanding of this singularity. With a rigorous combination of UT1–UTC and length of day (LOD) from VLBI and GPS, we showed that such a combination works very well and does not suffer from the systematic effects present in the GPS-derived LOD values. By means of wavelet analyses and the formal errors of the estimates, we explain this important result. The same holds for the combination of nutation offsets and rates. The local geodetic ties between GPS and VLBI antennas play an essential role within the inter-technique combination. Several studies already revealed non-negligible discrepancies between the terrestrial measurements and the space-geodetic solutions. We demonstrate to what extent these discrepancies propagate into the combined EOP solution.  相似文献   

19.
 At the present time, the daily VLBI observations on the Westford-Wettzell baseline is the only continually running VLBI project for studies of high-frequency Earth rotation variations. An analysis of this experiment with regard to the potential errors in the atmospheric delay model and in adopted celestial and terrestrial reference frames is presented in the paper. A new VLBI geometric delay model is applied and an algorithm for global adjustment for this specific single-baseline VLBI developed. The results over three years show discrepancies at the milliarcsecond level between the daily observations and the adopted atmospheric model as well as the combined celestial reference frame. A significant number of these discrepancies are removed by the global adjustment. Received: 19 August 1996; Accepted: 13 September 1996  相似文献   

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