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1.
差分码偏差(DCB)作为电离层建模和导航定位中一项重要的误差源,对其进行估计求解至关重要. 为提高北斗卫星导航系统(BDS) DCB估计和电离层建模精度,提出了一种综合高度角、卫地距和测站纬度多因素的随机模型,并对比分析了不同随机模型对BDS DCB估计和电离层垂直总电子含量(VTEC)建模精度的影响. 结果表明:不同随机模型对卫星端DCB解算产生约0.2 ns差异. 相较于高度角随机模型,采用高度角、卫地距组合模型测站DCB估计精度平均提高0.13 ns,电离层建模精度提高了约0.2 TECU. 新提出的随机模型,在低纬度测站DCB解算精度上差于高度角模型和高度角、卫地距组合模型,但在高纬度测站DCB解算结果上更优,且对电离层VTEC建模精度提升效果明显,与前两种随机模型相比分别提升了0.88 TECU和0.68 TECU. 相似文献
2.
Ionospheric electron density observed by FORMOSAT-3/COSMIC over the European region and validated by ionosonde data 总被引：4，自引：0，他引：4
Andrzej Krankowski Irina Zakharenkova Anna Krypiak-Gregorczyk Irk I. Shagimuratov Pawel Wielgosz 《Journal of Geodesy》2011,85(12):949-964
This research is motivated by the recent IGS Ionosphere Working Group recommendation issued at the IGS 2010 Workshop held
in Newcastle, UK. This recommendation encourages studies on the evaluation of the application of COSMIC radio occultation
profiles for additional IGS global ionosphere map (GIM) validation. This is because the reliability of GIMs is crucial to
many geodetic applications. On the other hand, radio occultation using GPS signals has been proven to be a promising technique
to retrieve accurate profiles of the ionospheric electron density with high vertical resolution on a global scale. However,
systematic validation work is still needed before using this powerful technique for sounding the ionosphere on a routine basis.
In this paper, we analyze the properties of the ionospheric electron density profiling retrieved from COSMIC radio occultation
measurements. A comparison of radio occultation data with ground-based measurements indicates that COSMIC profiles are usually
in good agreement with ionosonde profiles, both in the F2 layer peak electron density and the bottom side of the profiles.
For this comparison, ionograms recorded by European ionospheric stations (DIAS network) in 2008 were used. 相似文献
3.
4.
The ionospheric shell height has an impact on the estimated differential code bias (DCB) and total electron content (TEC) obtained by global navigation satellite system (GNSS) data, especially for a single site. However, the shell height is generally considered as a fixed value. Based on data from the international GNSS service (IGS), we propose the concept of optimal ionospheric shell height, which minimizes |ΔDCB| when compared to the DCB provided by Center for Orbit Determination in Europe (CODE). Based on the data from five IGS stations at high, middle, and low latitudes during the time 2003–2013, we investigate the variation in the optimal ionospheric shell height and its relation with the solar activity. Results indicate that the relation between the mean of the optimal ionospheric shell height and the latitude is N-shaped. At the three stations at midlatitude, the mean value almost increases linearly with the latitude. The optimal ionospheric shell heights show 11-year and 1-year periods. The influences of the solar activity are related to the means of the optimal ionospheric shell height during the time 2003–2013. The slope of the linear fitting decreases with the mean value. Using the data from 2003 to 2013, we estimate the daily optimal ionospheric shell heights for 2014 by using the Fourier fitting method and then calculate the daily average of ΔDCB of the observed satellites by comparing to CODE results. The statistical results of the daily average in 2014 show that the optimal ionospheric shell height is much better than the fixed one. From the high-latitude station to the low-latitude station, the improvements in the mean value are about 75, 92, 96, 50, and 88% and the root-mean-squares are reduced by about 0.16, 2.09, 2.01, 1.01, and 0.02 TECu, respectively. 相似文献
5.
Canada has recently faced two geodetic problems. Existing control on land must be rapidly upraged for resource development
and for the coming redefinition of North American networks. Geodetic methods of managing territorial and lease boundaries
in the offshore region are required. A series of developments in Doppler Satellite techniques begun in 1968 have contributed
to the solution of both these problems. Today these developments have resulted in a Canadian-made receiver, permanent Canadian
tracking stations, a primary geodetic network of about 200 Doppler points, major Doppler processing software systems, and
the routine use of Doppler points, major Doppler processing software systems, and the routine use of Doppler positioning for
land surveying, drill rig positioning and precise navigation. The accuracy of Doppler positioning has been improved from 100
m in 1968 to better than 1 m in 1975. These developments have applications in other nations than Canada. 相似文献
6.
与验潮站技术相比,岸基全球导航卫星定位系统干涉反射技术(GNSS-IR)海面测高成本较低,且其观测量不受地壳沉降的影响,并可利用目前已有的沿海岸GNSS固定站提供的数据反演海面高度。目前常用观测量为大地测量型GNSS接收机给出的信噪比(SNR)值,然而,早期很多GNSS设备的输出文件中都不包含该值,导致无法利用它们研究海面高度长期变化趋势。但经典的码伪距和载波相位观测值中,同样包含着GNSS-IR测高信息。本文分别引入单频码伪距和单频载波相位的组合,以及单频码伪距和双频载波相位的组合GNSS两种观测值的组合实现了岸基海面测高。本文采用模拟数据证明了基于前一组合的GNSS-IR测高精度受到电离层延迟残差的影响,而后一种组合可避免该误差项的影响。为验证两种组合方法的有效性,在山东威海一海上栈桥上开展了试验,采集了全球定位系统(GPS)和北斗卫星导航系统(BDS)的观测数据,并处理得到了海面测高信息。最后,将反演结果与26 GHz雷达高度计的观测值进行了比较分析,发现二者具有较好的一致性,相关系数均优于85%。试验结果表明:两种码伪距和载波相位组合法均可用于GNSS-IR测高。另外,由于当前GNSS-IR测高受多种误差项影响,导致反演精度较低,使得后一种组合在避免电离层延迟残差方面的优越性并没有明显体现。本文组合方法的引入,增加了海面高度反演方法的多样性,提升了GNSS-IR测高技术的应用空间。 相似文献
7.
The network-based GPS technique provides a broad spectrum of corrections to support RTK (real-time kinematic) surveying and
geodetic applications. The most important among them are the ionospheric corrections generated in the reference network. The
accuracy of these corrections depends upon the ionospheric conditions and may not always be sufficient to support ambiguity
resolution (AR), and hence accurate GPS positioning. This paper presents the analyses of the network-derived ionospheric correction
accuracy under extremely varying – quiet and stormy – geomagnetic and ionospheric conditions. In addition, the influence of
the correction accuracy on the instantaneous (single-epoch) and on-the-fly (OTF) AR in long-range RTK GPS positioning is investigated,
and the results, based on post-processed GPS data, are provided. The network used here to generate the ionospheric corrections
consists of three permanent stations selected from the Ohio Continuously Operating Reference Stations (CORS) network. The
average separation between the reference stations was ∼200 km and the test baseline was 121 km long. The results show that,
during the severe ionospheric storm, the correction accuracy deteriorates to the point when the instantaneous AR is no longer
possible, and the OTF AR requires much more time to fix the integers. The analyses presented here also outline the importance
of the correct selection of the stochastic constraints in the rover solution applied to the network-derived ionospheric corrections. 相似文献
8.
针对电离层延迟误差目前是GNSS导航定位精度最重要误差源的现状,通过GNSS参考站或跟踪站实测数据计算电子总含量值,建立区域电离层模型,监测区域电离层变化,进而找到削弱或消除电离层延迟误差影响方法。利用曲面拟合实现建模,在模型的建立过程中通过对不同的模型阶数进行设置,对比不同情况下的模型精度,从而确定特定区域内最佳数据采样间隔及阶数设置,并在最佳阶数设置情况下,比较了预报不同时段的精度,进而对延迟量预报问题进行探讨,得出一些有益结论。可以通过该模型单独解算流动站站点的实时电离层延迟信息,这对多基站CORS的站间距离选择和单基站CORS基准站和流动站之间距离设计,尤其对提高单频接收机以及GIS产品用户的定位精度和差分模型的覆盖范围都具有实际参考意义。 相似文献
9.
S. Pireaux P. Defraigne L. Wauters N. Bergeot Q. Baire C. Bruyninx 《GPS Solutions》2010,14(3):267-277
In high-precision geodetic time and frequency transfer, which requires precise modeling of code and carrier phase GPS data,
the ionosphere-free combinations P
3
and L
3
of the codes and carrier phases, made on the two GPS frequencies, are used to remove the first-order ionospheric effect.
We quantify the impact of the residual second- and third-order ionospheric effects on geodetic time and frequency transfer
solutions for continental and intercontinental baselines. All time transfer computations are done using the ATOMIUM software,
developed at the Royal Observatory of Belgium. In order to avoid contamination by some imperfect modeling of the second- and
third-order ionospheric effects in the satellite clock products, only single-difference, common-view processing is used, based
on code and carrier phase measurements. The results are shown for weak and strong solar activity, as well as for particular
epochs of ionospheric storms. Second-order ionospheric delays can lead to corrections up to about 10 ps in the common-view
clock solution of intercontinental baselines with very different longitudes. However, realistic values of the geomagnetic
field in the ionosphere are required to assess the amplitude of second-order ionospheric effects in time and frequency transfer
during an ionospheric storm. 相似文献
10.
针对如何有效控制、改正甚至消除不同区域与时段的电离层高阶项延迟对全球导航卫星系统定位结果产生的影响,该文选取了不同区域内有代表性的IGS基准站1999—2003年的观测数据进行解算,并详细分析了各测站坐标受高阶电离层延迟影响的规律。在此基础上,总结出测站的高阶项改正与测站区域地理位置的关系,并探究产生这种影响的原因。最后从全球的角度研究了电离层高阶项改正对基准站坐标的影响。结果表明,要获得高精度的定位结果,需要顾及高阶电离层延迟的影响,尤其是在赤道以及地球两极区域的精密定位,此外,需要顾及电离层变化活跃期的影响。 相似文献
11.
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
12.
Improvement in PWV estimation from GPS due to the absolute calibration of antenna phase center variations 总被引：1，自引：0，他引：1
Climatology of column-integrated atmospheric water vapor over Spain has been carried out by means of three techniques: soundings,
sun photometers and GPS receivers. Comparing data from stations equipped with more than one of these instruments, we found
that a large discontinuity occurred on November 6, 2006, in the differences between the data series from GPS receivers and
those from the other two techniques. Prior to that date, the GPS data indicate a wet bias of 2–3 mm for all stations when
compared with sounding or photometer data, whereas after that date this bias practically reduces to zero. The root mean square
error also decreases about half of its value. On November 6, 2006, the International GNSS Service adopted an absolute calibration
model for the antennas of the GPS satellites and receivers instead of the relative one. This change is expected to be an improvement,
increasing the accuracy of station position determination and consequently benefiting post-processing products such as zenith
total delay from which the atmospheric water vapor content is calculated. 相似文献
13.
GNSS-MR技术用于潮位变化监测分析 总被引：2，自引：1，他引：1
潮位变化的高精度监测一直是全球海平面观测系统、海洋环流和全球气候变化研究领域关注的热点问题之一。随着GNSS研究与应用的不断深入,近年来基于多路径效应的GNSS-MR技术已逐步成为一种新兴的遥感手段,即利用测量型GNSS站进行地表环境(植被、土壤湿度、雪深、潮位、火山活动等)监测。通过分析由多路径引起岸基GNSS站SNR值的变化特性,本文给出了基于SNR观测值的GNSS-MR技术监测潮位变化的反演原理。利用布设在美国华盛顿州Friday Harbor海港岸边的CORS站SC02实测观测数据对潮位变化监测进行了反演分析,并与该站相距359 m的验潮站数据进行了对比分析,两者较差均值约为10 cm左右,两者的相关系数均优于0.98。试验结果分析表明基于岸基CORS站的GNSS-MR技术在一定程度上可用于实时、连续的潮位变化监测,同时也说明岸基CORS站在一定程度上可作为验潮站的补充,进一步拓展GNSS在海洋遥感领域的应用范围。 相似文献
14.
Peter F. MacDoran 《Journal of Geodesy》1979,53(2):117-138
The satellites of the Global Positioning System (GPS) offer an important new geodetic resource making possible a highly accurate
portable radio geodetic system. A concept called SERIES (Satellite Emission Radio Interferometric Earth Surveying) makes use
of GPS radio transmissions without any satellite modifications. By employing the technique of very long baseline interferometry
(VLBI) and its calibration methods, 0.5 to 3 cm three dimensional baseline accuracy can be achieved over distances of 2 to
200 km respectively, with only 2 hours of on-site data acquisition. The use of quasar referenced ARIES Mobile VLBI to establish
a sparse fundamental control grid will provide a basis for making SERIES GPS measurements traceable to the time-invariant
quasar directions. Using four SERIES stations deployed at previously established ARIES sites, allows the GPS satellite apparent
positions to be determined. These apparent positions then serve as calibrations for other SERIES stations at unknown locations
to determine their positions in a manner traceable to the quasars. Because this proposed radio interferometric configuration
accomplishes its signal detection by cross-correlation, there is no dependence upon knowledge of the GPS transmitted waveforms
which might be encrypted. Since GPS radio signal strengths are 105 stronger than quasar signals, a great reduction in telecommunications sophistication is possible which will result in an
order of magnitude less cost for a SERIES GPS station compared to a quasar based mobile VLBI system. The virtually all-weather
capability of SERIES offers cost-effective geodetic monitoring with applications to crustal dynamics and earthquake research. 相似文献
15.
针对现有内插模型是否能够满足长距离稀疏参考站下电离层误差内插精度要求的问题,以线性内插模型、距离相关内插模型作为研究对象,首先结合误差传播定律从理论上比较两种内插模型对参考站间电离层延迟估值误差的抗差性;然后选取多组距主参考站不同距离的实例数据,分析比较模型内插精度的变化规律。实例结果表明:LIM模型内插精度分布较均匀,且优于DIM模型;对比中长距离(100 km),在长距离稀疏参考站下,模型内插精度明显降低,特别是对于电离层误差波动范围较大的卫星,其内插偏差超过±3 cm的达到50%以上。 相似文献
16.
Application of the TaiWan Ionospheric Model to single-frequency ionospheric delay corrections for GPS positioning 总被引：2，自引：2，他引：0
The performance of a three-dimensional ionospheric electron density model derived from FormoSat3/COSMIC GPS Radio Occultation measurements, called the TaiWan Ionosphere Model (TWIM), in removing the ionospheric delays in single-frequency pseudorange observations is presented. Positioning results using TWIM have been compared with positioning results using other ionospheric models, such as the Klobuchar (KLOB) and the global ionospheric model (GIM). C/A code pseudoranges have been observed at three International GPS Service reference stations that are representative of mid-latitude (BOR1 and IRKJ) and low-latitude (TWTF) regions of the ionosphere. The observations took place during 27 geomagnetically quiet days from April 2010 to October 2011. We perform separate solutions using the TWIM, KLOB, GIM ionospheric models and carry out a solution applying no ionospheric correction at all. We compute the daily mean horizontal errors (DMEAN) and the daily RMS (DRMS) for these solutions with respect to the published reference station coordinates. It has demonstrated that TEC maps generate using the TWIM exhibit a detailed structure of the ionosphere, particularly at low-latitude region, whereas the Klobuchar and the GIM only provide the basic diurnal and geographic features of the ionosphere. Also, it is shown that even for lower satellite elevations, the TWIM provides better positioning than the Klobuchar and GIM models. Specifically, using TWIM, the difference of the uncorrected solution (no ionospheric correction), and the other solutions, relative to the uncorrected solution, is 45 % for the mean horizontal error (DMEAN) and 42 % for the horizontal root-mean-square error (DRMS). Using Klobuchar and GIM, the percent for DMEAN only reaches to about 12 % and 3 %, while the values for the DRMS are only 12 and 4 %, respectively. In the vertical direction, all models have a percentage of about 99 and 70 % for the mean vertical error (VMEAN) and vertical root-mean-square error (VRMS), respectively. These percentages show the greater impact of TWIM on the ionospheric correction compared to the other models. In at least 40 % of the observed days and across all stations, TWIM has the smallest DMEAN, VMEAN, DRMS, and VRMS daily values. These values reach 100 % at station TWTF. This shows the overall performance of TWIM is better than the Klobuchar and GIM. 相似文献
17.
Precise GPS Positioning by Applying Ionospheric Corrections from an Active Control Network 总被引：2，自引：1，他引：1
In this article, initial results are presented of a method to improve fast carrier phase ambiguity resolution over longer
baselines (with lengths up to about 200 km). The ionospheric delays in the global positioning system (GPS) data of these long
baselines mainly hamper successful integer ambiguity resolution, a prerequisite to obtain precise positions within very short
observation time spans.
A way to correct the data for significant ionospheric effects is to have a GPS user operate within an active or permanently
operating network use ionospheric estimates from this network. A simple way to do so is to interpolate these ionospheric estimates
based on the expected spatial behaviour of the ionospheric delays. In this article such a technique is demonstrated for the
Dutch Active Control Network (AGRS.NL). One hour of data is used from 4 of the 5 reference stations to obtain very precise
ionospheric corrections after fixing of the integer ambiguities within this network. This is no problem because of the relatively
long observation time span and known positions of the stations of the AGRS.NL. Next these interpolated corrections are used
to correct the GPS data from the fifth station for its ionospheric effects. Initial conclusions about the performance of this
technique are drawn in terms of improvement of integer ambiguity resolution for this baseline. ? 1999 John Wiley & Sons, Inc. 相似文献
18.
利用单个基准站提供的改正信息对流动站的单频观测值数据进行改正,同时引入电离层参数进行实时电离层延迟估计,进行单频精密单点定位（PPP）计算。相比传统的单频PPP方法,本文方法对单频PPP的收敛速度和定位精度都有很大的提高,定位精度优于2cm,且受基准站距离的影响较小。 相似文献
19.
GPS tomography in the polar cap: comparison with ionosondes and in situ spacecraft data 总被引：2，自引：1，他引：1
Dimitry Pokhotelov P. T. Jayachandran Cathryn N. Mitchell John W. MacDougall Michael H. Denton 《GPS Solutions》2011,15(1):79-87
Tomographic 4D reconstructions of ionospheric anomalies appearing in the high-latitude polar cap region are compared with
plasma density measurements by digital ionosonde located near the north magnetic pole at Eureka station and with in situ plasma
measurements on-board DMSP spacecraft. The moderate magnetic storm of 14–17 October 2002 is taken as an example of a geomagnetic
disturbance which generates large-scale ionospheric plasma anomalies at mid-latitudes and in the polar cap region. Comparison
of the GPS tomographic reconstructions over Eureka station with the ionosonde measurements of the F layer peak densities indicates
that the GPS tomography correctly predicts the time of arrival and passage of the ionospheric tongue of ionization over the
magnetic pole area, although the tomographic technique appears to under-estimate the value of F peak plasma density. Comparison
with the in situ plasma measurements by the DMSP SSIES instruments shows that the GPS tomography correctly reproduces the
large-scale spatial structure of ionospheric anomalies over a wide range of latitudes from mid-latitudes to the high-latitude
polar cap region, though the tomographic reconstructions tend to over-estimate the density of the topside ionosphere at 840 km
DMSP orbit. This study is essential for understanding the quality and limitations of the tomographic reconstruction techniques,
particularly in high-latitude regions where GPS TEC measurements and other ionospheric data sources are limited. 相似文献
20.
根据电离层高阶项改正模型,确定了高阶项延迟对不同GPS观测量的影响量。根据IERS协议2010推荐的最新模型,对全球均匀分布的104个IGS基准站数据进行了重新处理,研究了电离层高阶项延迟(二、三阶项)对坐标参考框架实现及测站坐标的影响,量化了不同地磁模型下的高阶项改正影响变化。结果表明,电离层延迟高阶项改正对参考框架原点有较大影响,犣方向的平移可达20mm,犡、犢方向的平移所受的影响相对较小,大部分维持在5mm以下;电离层高阶项延迟会引起测站坐标变化的区域性偏移现象;地磁模型的不同会导致参考框架原点犣方向有着约10mm的变化,在局部区域也会引起显著的测站坐标变化差异。最后对电离层高阶项改正的影响结果进行了分析与讨论。 相似文献