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1.
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   

2.
In this paper, a new geometry index of very long baseline interferometry (VLBI) observing networks, the volume of network V, is examined as an indicator of the errors in the Earth orientation parameters (EOP) obtained from VLBI observations. It has been shown that both EOP precision and accuracy can be well described by the power law σ = aV c in a wide range of the network size from domestic to global VLBI networks. In other words, as the network volume grows, the EOP errors become smaller following a power law. This should be taken into account for a proper comparison of EOP estimates obtained from different VLBI networks. Thus, performing correct EOP comparison allows us to investigate accurately finer factors affecting the EOP errors. In particular, it was found that the dependence of the EOP precision and accuracy on the recording data rate can also be described by a power law. One important conclusion is that the EOP accuracy depends primarily on the network geometry and to lesser extent on other factors, such as recording mode and data rate and scheduling parameters, whereas these factors have a stronger impact on the EOP precision.  相似文献   

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4.
对VLBI数据库进行了详细的研究,揭示了其结构和数据存取格式,给出了数据库信息列表,并对数据库管理程序进行了说明。  相似文献   

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6.
本文结合流动VLBI参加的"地壳运动观测网络工程"和"探月工程",从建立和维护我国地心参考框架和深空探测两个角度讨论了流动VLBI站址的选择、以及所选站址对我国VLBI观测网的改善。提出了将流动VLBI站设在海南,这样既增加了南北基线长度,也扩大了可观测射电源的范围,同时在建立和维持我国地心参考框架方面也是较好的选择。  相似文献   

7.
本文系统地研究了VLBI天体测量和大地测量数据处理软件系统(CALC/SOLVK)。利用最新VLBI观测资料(1993年~1994年)对各类天文地球动力学参数进行了精密的测定和研究。  相似文献   

8.
VLBI技术的发展与展望   总被引:2,自引:0,他引:2  
至今,VLBI技术经过迅猛发展,先后经历了以下三个发展阶段:传统VLBI、实时和准实时VLBI以及空间VLBI。本文分别介绍这三种VLBI技术的定义及其特点,通过对比分析其优缺点,展望VLBI技术的未来发展。  相似文献   

9.
We have used Very Long Baseline Interferometry (VLBI) data to compute the site coordinates and constant velocity components for 29 fixed antenna sites and 25 mobile sites. The three singularities which occur in the adjustment with respect to the rotation of the system have been resolved by a constraint holding the net rotation of seven fixed antennas, distributed on the stable portions of four of the geologic plates, to the net rotation for these sites as defined by the NNR-NUVEL1 no net rotation model. In order to achieve a minimally constrained adjustment of this type we have found it necessary to use a new adjustment procedure in which we solve for the coordinates of each site at the weighted mean epoch of all the observations involving that site.Using the results of the above solution we have computed the departure for each site from the NNR-NUVEL1 rigid plate model. These departures show that the transition zone in western North America from the region of rigidity to the plate boundary is at least 400 km wide, in general agreement with Ward (1988,1990).  相似文献   

10.
流动VLBI观测频率窗口的选择   总被引:3,自引:0,他引:3  
为即将启动的流动VLBI系统选取了频率窗口, 并对我国VLBI站所组成基线的系统性能和观测精度进行了估计。结果表明该频窗的选取是可行的。  相似文献   

11.
讨论了流动VLBI观测计划表的编制过程;对射电源的选取、系统性能、观测时间的确定以及观测计划文件的生成等问题进行了研究.  相似文献   

12.
本文以太阳系质心参考系为基础推导了VLBI时延和引力延迟的后牛顿表达式;讨论了各天体对VLBI时延的影响量级及其作用范围;并根据地心参考系与太阳系质心参考系的坐标转换关系,给出了地心参考系中的VLBI观测模型。建议采用(25)式和(16)式作为VLBI时延和引力延迟改正的计算公式。  相似文献   

13.
本文探讨了空间VLBI较差测量的基本原理和数学模型,对类星体和脉冲星的较差测量进行了分析,列出了RADIOASTRON空间VLBI站可能观测到的脉冲星。  相似文献   

14.
讨论了流动VLBI观测计划表的编制过程;对射电源的选取、系统性能、观测时间的确定以及观测计划文件的生成等问题进行了研究。  相似文献   

15.
Correlation algorithms for geodetic very long baseline interferometry (VLBI) can now be effectively implemented on parallel computers of modest size. We have undertaken a detailed comparison of the output from a trusted geodetic correlator, one that has supported global geodetic VLBI observations for many years, with the output of a software correlator implemented on a small parallel computing cluster. We show that the correlator outputs agree closely, within expected error bounds, after accounting for the differences in the adopted geometric delay models, and therefore that use of the software correlator is feasible for geodetic VLBI processing, as a first step toward routine geodetic data processing. Recent developments in software correlation for geodesy are discussed, including the possibility of real-time processing options.  相似文献   

16.
参考《全球定位系统(GPS)测量规范》之附录G归心元素测定,采用测GPS的方法,对固置在昆明的流动VLBI站进行了归心计算,在得到流动VLBI用GPS技术所测量的地心坐标同时,指出了参考文献[1]中存在的矛盾与错误,并结合实际应用,给出了一组实用的计算公式。  相似文献   

17.
VLBI,SVLBI技术用于月球探测器定位的理论模型   总被引:1,自引:0,他引:1  
"嫦娥一号"为我国的深空探测拉开了序幕,高端的VLBI以及SVLBI技术在我国探测器定位领域中的地位是其他技术无可取代的.以VLBI技术为基础,分别列出利用地而VLBI和空间VLBI观测量两种观测确定月球探测器位置的理论模型,并整理得到间接平差的误差方程.  相似文献   

18.
本文介绍了流动VLBI终端系统的技术改造与升级情况以及MK5A数据系统的构成与工作原理,论述了实现BBC系统本振步长、BBC滤波器带宽和带宽增益补偿以及流动VLBI数据系统等方面的技术改造与升级的原理和方法,最后介绍了应用结果。  相似文献   

19.
针对我国 VL BI观测网对射电源的特殊要求 ,给出了现有备选射电源的列表和天球分布图 ,提出了扩充备选射电源数量的必要性。结合 2 0 0 0年 1月“上海 -昆明基线”试观测 ,在原有的 12个备选射电源的基础上 ,又增选了 4个。观测及计算结果显示 ,12个备选源中 ,有 11个的信噪比和相关流量都很好 ,1个勉强能用 ;4个增选的源中 ,有 3个达到指标 ,应放入以后的备选源中。  相似文献   

20.
European geodetic very long baseline interferometry (VLBI) sessions (also known as EUROPE sessions) have been carried out on a regular basis for the past 15 years to study relative crustal motions within Europe. These sessions are based on observations of extragalactic radio sources, which serve as distant fiducial marks to establish an accurate and stable celestial reference frame for long-term geodetic measurements. The radio sources, however, are not always point-like on milliarcsecond scales, as VLBI imaging has revealed. In this work, we quantify the magnitude of the expected effect of intrinsic source structure on geodetic bandwidth synthesis delay VLBI measurements for a subset of 14 sources regularly observed during the EUROPE sessions. These sources have been imaged at both X-band (8.4 GHz) and S-band (2.3 GHz) based on dedicated observations acquired with the European VLBI Network (EVN) in November 1996. The results of this calculation indicate that the reference source 0457+024 causes significant structural effects in measurements obtained on European VLBI baselines (about 10 picoseconds on average), whereas most of the other sources produce effects that are only occasionally larger than a few picoseconds. Applying the derived source structure models to the data of the EUROPE5-96 session carried out at the same epoch as the EVN experiment shows no noticeable changes in the estimated VLBI station locations.  相似文献   

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