共查询到19条相似文献，搜索用时 829 毫秒
1.
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
2.
本文采用最近获得的ＶＬＢＩ基线变化率，解算了全球５０个ＶＬＢＩ站的站速度。通过对ＶＬＢＩ台站构造稳定性的分析，用位于板块稳定地区台站的站速度求解了欧亚（ＥＵＲＡ）、北美（ＮＯＡＭ）和太平洋（ＰＣＦＣ）三个主要板块之间的相对运动欧拉矢量，这是完全基于ＶＬＢＩ数据导出的板块运动模型，称为ＶＰ－ＭＭ１。通过ＶＰＭＭ１与地学板块运动模型的比较，分析了板块运动的稳定性，得出了几点初步结论。 相似文献
3.
本文概述了中性大气层对ＶＬＢＩ时延观测值的影响，给出了计算这一影响的基本方法和各种映射函数模型并综合比较了它们的特性和适用范围，介绍了这些模型在ＶＬＢＩ大地测量数据处理软件ＸＰＶＳ中的实现。通过对实际观测数据处理所获各种模型结果的比较和分析，表明在与目前国标上标准ＶＬＢＩ解一致的条件下，最佳映射函数模型为ＣｆＡ２．２干气／Ｃｈａｏ湿汽模型；Ｉｆａｄ和ＭＴＴ大气模型的精度高于目前使用的ＣｆＡ２．２／ 相似文献
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5.
全球定位系统（ＧＰＳ）及其在高等级道路勘测中的应用ＧＬＯＢＡＬＰＯＳＩＴＩＯＮＩＮＧＳＹＳＴＥＭ（ＧＰＳ）ＡＮＤＩＴＳＡＰＰＬＩＣＡＴＩＯＮＴＯＨＩＧＨ－ＧＲＡＤＥＲＯＡＤＲＥＣＯＮＮＡＩＳＳＡＮＣＥＳＵＲＶＥＹ姚连璧（同济大学测量与国土信息工程系,... 相似文献
6.
本文例举了ＶＬＢＩ技术的现状与发展，阐述了该技术在研究全球变化中的贡献以及中国参与国际ＶＬＢＩ大地测量的计划。 相似文献
7.
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
8.
植被结构及太阳／观测角度对NDVI的影响 总被引：1，自引：0，他引：1
在文献［１］中作者建立了计算多组分植被方向反射系数（ＢＲＦ）的综合解析模型。本文采用该模型研究植被空间结构对常用的归一化植被指数（ＮＤＶＩ）的影响，文中讨论了ＮＤＶＩ与叶（或植被其它组分）角分布（ＬＡＤ）、植被组分（如叶片）的特征尺度和它们在空间的散布方式，以及非叶器官面积在总面积中所占比例间的依赖关系，同时给出了ＮＤＶＩ随太阳／观测角度的变化情况。结果表明即使在叶面积指数（ＬＡＩ）固定不变时，冠层结构及植被组分光学性质的空间非均匀性对ＮＤＶＩ的大小及角分布也有十分显著的影响。通常ＮＤＷ随角度的变化是很大的，如果植被不同组分的光学性质差异很大，且事先不知道它们的空间散布方式时，那么利用ＤＮＶＩ就无法准确地估算出ＬＡＩ。但是对于组分随机分布的植被，利用远离“热点”区域的光谱资料可以使冠层其它结构参数的影响减至最小。 相似文献
9.
对VLBI测地数据处理软件的改进 总被引：3，自引：0，他引：3
对国际上目前通用的ＶＬＢＩ数据处理软件包ＯＣＣＡＭ Ｖ３．３进行了一系列的改进,并对９７,９８年的几次观测资料进行了处理。结果证明,改进是必须的、成功的。改进后的软件解算更自动化,且简化了求解参数。 相似文献
10.
作者曾经利用扫描矢量化软件Ｉ／ＲＡＳＢ和Ｉ／ＧＥＯＶＥＣ在ＧＩＳ和数字地图中进行了各种各样的应用研究。本文着重介绍Ｉ／ＲＡＳＢ和Ｉ／ＧＥＯＶＥＣ等在ＧＩＳ和地图数字化中的应用方法，包括矢量文件和光栅文件。 相似文献
11.
O. Titov 《Journal of Geodesy》2007,81(6-8):455-468
This paper evaluates the effect of the accuracy of reference radio sources on the daily estimates of station positions, nutation
angle offsets, and the estimated site coordinates determined by very long baseline interferometry (VLBI), which are used for
the realization of the international terrestrial reference frame (ITRF). Five global VLBI solutions, based on VLBI data collected
between 1979 and 2006, are compared. The reference solution comprises all observed radio sources, which are treated as global
parameters. Four other solutions, comprising different sub-sets of radio sources, were computed. The daily station positions
for all VLBI sites and the corrections to the nutation offset angles were estimated for these five solutions. The solution
statistics are mainly affected by the positional instabilities of reference radio sources, whereas the instabilities of geodetic
and astrometric time-series are caused by an insufficient number of observed reference radio sources. A mean offset of the
three positional components (Up, North, East) between any two solutions was calculated for each VLBI site. From a comparison
of the geodetic results, no significant discrepancies between the respective geodetic solutions for all VLBI sites in the
Northern Hemisphere were found. In contrast, the Southern Hemisphere sites were more sensitive to the selected set of reference
radio sources. The largest estimated mean offset of the vertical component between two solutions for the Australian VLBI site
at Hobart was 4 mm. In the worst case (if a weak VLBI network observed a limited number of reference radio sources) the daily
offsets of the estimated height component at Hobart exceeded 100 mm. The exclusion of the extended radio sources from the
list of reference sources improved the solution statistics and made the geodetic and astrometric time-series more consistent.
The problem with the large Hobart height component offset is magnified by a comparatively small number of observations due
to the low slewing rate of the VLBI dish (1°/ s). Unless a minimum of 200 scans are performed per 24-h VLBI experiment, the
daily vertical positions at Hobart do not achieve 10 mm accuracy. Improving the slew rate at Hobart and/or having an increased
number of new sites in the Southern Hemisphere is essential for further improvement of geodetic VLBI results for Southern
Hemisphere sites. 相似文献
12.
13.
New VLBI2010 scheduling strategies and implications on the terrestrial reference frames 总被引：1，自引：1，他引：0
Jing Sun Johannes Böhm Tobias Nilsson Hana Krásná Sigrid Böhm Harald Schuh 《Journal of Geodesy》2014,88(5):449-461
In connection with the work for the next generation VLBI2010 Global Observing System (VGOS) of the International VLBI Service for Geodesy and Astrometry, a new scheduling package (Vie_Sched) has been developed at the Vienna University of Technology as a part of the Vienna VLBI Software. In addition to the classical station-based approach it is equipped with a new scheduling strategy based on the radio sources to be observed. We introduce different configurations of source-based scheduling options and investigate the implications on present and future VLBI2010 geodetic schedules. By comparison to existing VLBI schedules of the continuous campaign CONT11, we find that the source-based approach with two sources has a performance similar to the station-based approach in terms of number of observations, sky coverage, and geodetic parameters. For an artificial 16 station VLBI2010 network, the source-based approach with four sources provides an improved distribution of source observations on the celestial sphere. Monte Carlo simulations yield slightly better repeatabilities of station coordinates with the source-based approach with two sources or four sources than the classical strategy. The new VLBI scheduling software with its alternative scheduling strategy offers a promising option with respect to applications of the VGOS. 相似文献
14.
In recent years, ocean tide loading displacements (OTLD) have been measured using the Global Positioning System (GPS) and
Very Long Baseline Interferometry (VLBI). This study assesses the accuracy of GPS measurements of OTLD by comparison with
VLBI measurements and estimates derived from numerical ocean tide models. A daily precise point positioning (PPP) analysis
was carried out on ∼11 years of GPS data for each of 25 sites that have previous OTLD estimates based on data from co-located
VLBI sites. Ambiguities were fixed to integer values where possible. The resulting daily estimates of OTLD, at eight principal
diurnal and semi-diurnal tidal frequencies, were combined to give GPS measurements of OTLD at each site. The 3D GPS and VLBI
measurements of OTLD were compared with estimates computed (by convolution with Green’s functions) from five modern ocean
tide models (CSR4.0, FES2004, GOT00.2, NAO99b and TPXO6.2). The GPS/model agreement is shown to be similar to the VLBI/model
agreement. In the important radial direction, the GPS/model misfit is shown to be smaller than the VLBI/model misfit for seven
of the eight tidal constituents; the exception being the K2 constituent. Fixing of GPS carrier-phase ambiguities to integer
values resulted in a marginal improvement to the GPS/model agreement. Statistically, it is shown there is no significance
to the difference between the fit of the GPS and VLBI measurements of OTLD to modelled values. Equally, differences in fit
of either the complete set of GPS or VLBI estimates to the five sets of model-derived values cannot be identified with statistical
significance. It is thus concluded that, overall, we cannot distinguish between GPS and VLBI measurements of OTLD, and that
at the global scale, present ocean tide models are accurate to within the current measurement noise of these techniques. 相似文献
15.
Ionospheric calibration of single frequency VLBI and GPS observations using dual GPS data 总被引：3，自引：1，他引：3
Summary The ionospheric effect is one of the main sources of error in Very Long Baseline Interferometry (VLBI) and Global Positioning System (GPS) high precision geodesy. Although the use of two frequencies allows the estimation of this effect, in some cases dual observations are not possible due to the available equipment or the type of observation. This paper presents the ionospheric calibration of single frequency VLBI and GPS observations based on the ionospheric electron content estimated from dual frequency GPS data. The ionospheric delays obtained with this procedure and the VLBI baseline length results have been compared with those obtained with dual frequency data. For the European geodetic VLBI baselines, both solutions agree at the 3–5 parts in 10–9 level. The noise introduced by the GPS-based calibration is in the order of 3 cm for the VLBI observables and of 10 cm for the GPS observables. 相似文献
16.
Height bias and scale effect induced by antenna gravitational deformations in geodetic VLBI data analysis 总被引：2，自引：2，他引：0
The impact of signal path variations (SPVs) caused by antenna gravitational deformations on geodetic very long baseline interferometry
(VLBI) results is evaluated for the first time. Elevation-dependent models of SPV for Medicina and Noto (Italy) telescopes
were derived from a combination of terrestrial surveying methods to account for gravitational deformations. After applying
these models in geodetic VLBI data analysis, estimates of the antenna reference point positions are shifted upward by 8.9
and 6.7 mm, respectively. The impact on other parameters is negligible. To simulate the impact of antenna gravitational deformations
on the entire VLBI network, lacking measurements for other telescopes, we rescaled the SPV models of Medicina and Noto for
other antennas according to their size. The effects of the simulations are changes in VLBI heights in the range [−3, 73] mm
and a net scale increase of 0.3–0.8 ppb. The height bias is larger than random errors of VLBI position estimates, implying
the possibility of significant scale distortions related to antenna gravitational deformations. This demonstrates the need
to precisely measure gravitational deformations of other VLBI telescopes, to derive their precise SPV models and to apply
them in routine geodetic data analysis. 相似文献
17.
James M. Anderson Georg Beyerle Susanne Glaser Li Liu Benjamin Männel Tobias Nilsson Robert Heinkelmann Harald Schuh 《Journal of Geodesy》2018,92(9):1023-1046
We performed Monte Carlo simulations of very-long-baseline interferometry (VLBI) observations of Earth-orbiting satellites incorporating co-located space-geodetic instruments in order to study how well the VLBI frame and the spacecraft frame can be tied using such measurements. We simulated observations of spacecraft by VLBI observations, time-of-flight (TOF) measurements using a time-encoded signal in the spacecraft transmission, similar in concept to precise point positioning, and differential VLBI (D-VLBI) observations using angularly nearby quasar calibrators to compare their relative performance. We used the proposed European Geodetic Reference Antenna in Space (E-GRASP) mission as an initial test case for our software. We found that the standard VLBI technique is limited, in part, by the present lack of knowledge of the absolute offset of VLBI time to Coordinated Universal Time at the level of microseconds. TOF measurements are better able to overcome this problem and provide frame ties with uncertainties in translation and scale nearly a factor of three smaller than those yielded from VLBI measurements. If the absolute time offset issue can be resolved by external means, the VLBI results can be significantly improved and can come close to providing 1 mm accuracy in the frame tie parameters. D-VLBI observations with optimum performance assumptions provide roughly a factor of two higher uncertainties for the E-GRASP orbit. We additionally simulated how station and spacecraft position offsets affect the frame tie performance. 相似文献
18.
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