Nothing Special   »   [go: up one dir, main page]

You seem to have javascript disabled. Please note that many of the page functionalities won't work as expected without javascript enabled.
 
 
Sign in to use this feature.

Years

Between: -

Subjects

remove_circle_outline
remove_circle_outline
remove_circle_outline

Journals

Article Types

Countries / Regions

Search Results (6)

Search Parameters:
Keywords = UNB3m model

Order results
Result details
Results per page
Select all
Export citation of selected articles as:
18 pages, 3142 KiB  
Article
Comprehensive Analysis of the Global Zenith Tropospheric Delay Real-Time Correction Model Based GPT3
by Jian Chen, Yushuang Jiang, Ya Fan, Xingwang Zhao and Chao Liu
Atmosphere 2023, 14(6), 946; https://doi.org/10.3390/atmos14060946 - 28 May 2023
Cited by 1 | Viewed by 1345
Abstract
To obtain a higher accuracy for the real-time Zenith Tropospheric Delay (ZTD), a refined tropospheric delay correction model was constructed by combining the tropospheric delay correction model based on meteorological parameters and the GPT3 model. The meteorological parameters provided by the Global Geodetic [...] Read more.
To obtain a higher accuracy for the real-time Zenith Tropospheric Delay (ZTD), a refined tropospheric delay correction model was constructed by combining the tropospheric delay correction model based on meteorological parameters and the GPT3 model. The meteorological parameters provided by the Global Geodetic Observing System (GGOS) Atmosphere and the zenith tropospheric delay data provided by Centre for Orbit Determination in Europe (CODE) were used as references, and the accuracy and spatial–temporal characteristics of the proposed model were compared and studied. The results show the following: (1) Compared with the UNB3m, GPT and GPT2w models, the accuracy and stability of the GPT3 model were significantly improved, especially the estimation accuracy of temperature, the deviation (Bias) of the estimated temperature was reduced by 90.60%, 32.44% and 0.30%, and the root mean square error (RMS) was reduced by 42.40%, 11.02% and 0.11%, respectively. (2) At different latitudes, the GPT3 + Saastamoinen, GPT3 + Hopfield and UNB3m models had great differences in accuracy and applicability. In the middle and high latitudes, the Biases of the GPT3 + Saastamoinen model and the GPT3 + Hopfield model were within 0.60 cm, and the RMS values were within 4 cm; the Bias of the UNB3m model was within 2 cm, and the RMS was within 5 cm; in low latitudes, the accuracy and stability of the GPT3 + Saastamoinen model were better than those of the GPT3 + Hopfield and UNB3m models; compared with the GPT3 + Hopfield model, the Bias was reduced by 22.56%, and the RMS was reduced by 5.67%. At different heights, the RMS values of the GPT3 + Saastamoinen model and GPT3 + Hopfield model were better than that of the UNB3m model. When the height was less than 500 m, the Biases of the GPT3 + Saastamoinen, GPT3 + Hopfield and UNB3m models were 3.46 cm, 3.59 cm and 4.54 cm, respectively. At more than 500 m, the Biases of the three models were within 4 cm. In different seasons, the Bias of the ZTD estimated by the UNB3m model had obvious global seasonal variation. The GPT3 + Saastamoinen model and the GPT3 + Hopfield model were more stable, and the values were within 5 cm. The research results can provide a useful reference for the ZTD correction accuracy and applicability of GNSS navigation and positioning at different latitudes, at different heights and in different seasons. Full article
(This article belongs to the Section Atmospheric Techniques, Instruments, and Modeling)
Show Figures

Figure 1

Figure 1
<p>Geographical distribution of the 25 IGS stations.</p>
Full article ">Figure 2
<p>Temperature (<b>a</b>), atmosphere pressure (<b>b</b>) and water vapor pressure (<b>c</b>) estimated by four non-measured meteorological parameter models compared with GGOS Atmosphere.</p>
Full article ">Figure 3
<p>Bias (<b>a</b>,<b>c</b>,<b>e</b>) and RMS (<b>b</b>,<b>d</b>,<b>f</b>) of four non-measured meteorological parameter models estimated using 25 IGS stations.</p>
Full article ">Figure 4
<p>The geographical distribution of the 297 selected IGS stations. (<b>Left</b>: station distribution map; <b>Right</b>: station elevation map).</p>
Full article ">Figure 5
<p>Bias of five models validated using ZTD data provided by CODE in 2019.</p>
Full article ">Figure 6
<p>RMS proportional distribution of the five models validated using ZTD data provided by CODE in 2019.</p>
Full article ">Figure 7
<p>Changes in Bias (<b>a</b>) and RMS (<b>b</b>) values of three models at different heights verified using ZTD data provided by CODE in 2019 (cm).</p>
Full article ">Figure 8
<p>Global distribution of Bias (<b>a</b>–<b>c</b>) and RMS (<b>d</b>–<b>f</b>) values of the three models.</p>
Full article ">Figure 9
<p>Bias time series of the three models using six IGS stations (the brackets indicate the longitude, latitude and height of each station) verified using ZTD data provided by CODE in 2019. ((<b>a</b>–<b>f</b>) represent the Bias of MRO1, WGTN, SCTB, PTGG, NICO, NRIL station).</p>
Full article ">
18 pages, 4637 KiB  
Article
Global Assessment of the GNSS Single Point Positioning Biases Produced by the Residual Tropospheric Delay
by Ling Yang, Jinfang Wang, Haojun Li and Timo Balz
Remote Sens. 2021, 13(6), 1202; https://doi.org/10.3390/rs13061202 - 22 Mar 2021
Cited by 8 | Viewed by 3119
Abstract
The tropospheric delay is one of the main error sources that degrades the accuracy of Global Navigation Satellite Systems (GNSS) Single Point Positioning (SPP). Although an empirical model is usually applied for correction and thereby to improve the positioning accuracy, the residual tropospheric [...] Read more.
The tropospheric delay is one of the main error sources that degrades the accuracy of Global Navigation Satellite Systems (GNSS) Single Point Positioning (SPP). Although an empirical model is usually applied for correction and thereby to improve the positioning accuracy, the residual tropospheric delay is still drowned in measurement noise, and cannot be further compensated by parameter estimation. How much this type of residual error would sway the SPP positioning solutions on a global scale are still unclear. In this paper, the biases on SPP solutions introduced by the residual tropospheric delay when using nine conventionally Zenith Tropospheric Delay (ZTD) models are analyzed and discussed, including Saastamoinen+norm/Global Pressure and Temperature (GPT)/GPT2/GPT2w/GPT3, University of New Brunswick (UNB)3/UNB3m, European Geostationary Navigation Overlay System (EGNOS) and Vienna Mapping Functions (VMF)3 models. The accuracies of the nine ZTD models, as well as the SPP biases caused by the residual ZTD (dZTD) after model correction are evaluated using International GNSS Service (IGS)-ZTD products from around 400 globally distributed monitoring stations. The seasonal, latitudinal, and altitudinal discrepancies are analyzed respectively. The results show that the SPP solution biases caused by the dZTD mainly occur on the vertical direction, nearly to decimeter level, and significant discrepancies are observed among different models at different geographical locations. This study provides references for the refinement and applications of the nine ZTD models for SPP users. Full article
(This article belongs to the Special Issue Advances in GNSS Data Processing and Navigation)
Show Figures

Graphical abstract

Graphical abstract
Full article ">Figure 1
<p>Distribution of global International GNSS Service (IGS) GPS sites.</p>
Full article ">Figure 2
<p>Mean and RMS between the IGS ZTD and the 9 models (saas+norm/GPT/GPT2/GPT2w/GPT3, EGNOS, UNB3, UNB3m, VMF3). To evaluate the model accuracies in different seasons, dZTD means and RMSs by different models are calculated and summarized by using each 7 day period’s data, as shown in <a href="#remotesensing-13-01202-f003" class="html-fig">Figure 3</a> and <a href="#remotesensing-13-01202-f004" class="html-fig">Figure 4</a>.</p>
Full article ">Figure 3
<p>Mean between the IGS ZTD and the 9 models (saas+norm/GPT/GPT2/GPT2w/GPT3, EGNOS, UNB3, UNB3m, VMF3) in different seasons.</p>
Full article ">Figure 4
<p>RMS between the IGS ZTD and the 9 models (saas+norm/GPT/GPT2/GPT2w/GPT3, EGNOS, UNB3, UNB3m, VMF3) in different seasons.</p>
Full article ">Figure 5
<p>Running time of the eight models (saas+norm/GPT/GPT2/GPT2w/GPT3, EGNOS, UNB3, UNB3m) (unit: μs).</p>
Full article ">Figure 6
<p>RMSs of the SPP solutions on the vertical direction produced by <span class="html-italic">dZTD</span> of the 9 models (saas+norm/GPT/GPT2/GPT2w/GPT3, EGNOS, UNB3, UNB3m, VMF3) in different seasons.</p>
Full article ">Figure 7
<p><span class="html-italic">dZTD</span> RMSs (upper panels) and RMSs of the SPP biases on the vertical direction (lower panels) generated by <span class="html-italic">dZTD</span> from saas+GPT (left panels) and UNB3 (right panels) models at globally distributed IGS stations (unit: cm).</p>
Full article ">Figure 8
<p>Means of the mapping coefficient between dZTD and the SPP biases on the vertical direction at globally distributed IGS stations.</p>
Full article ">Figure 9
<p>Number of stations at different latitude ranges.</p>
Full article ">Figure 10
<p>RMSs of the vertical SPP biases caused by dZTDs from the 9 models (saas+norm/GPT/GPT2/GPT2w/GPT3, EGNOS, UNB3, UNB3m, VMF3) at different latitude regions (unit: cm).</p>
Full article ">Figure 11
<p>RMSs of the vertical SPP biases by using the nine models at different heights (unit: cm).</p>
Full article ">
14 pages, 3318 KiB  
Article
Improved Zenith Tropospheric Delay Modeling Using the Piecewise Model of Atmospheric Refractivity
by Liu Yang, Jingxiang Gao, Dantong Zhu, Nanshan Zheng and Zengke Li
Remote Sens. 2020, 12(23), 3876; https://doi.org/10.3390/rs12233876 - 26 Nov 2020
Cited by 12 | Viewed by 2228
Abstract
As one of the atmosphere propagation delays, the tropospheric delay is a significant error source that should be properly handled in high-precision global navigation satellite system (GNSS) applications. We propose an improved zenith tropospheric delay (ZTD) modeling method whereby the piecewise model of [...] Read more.
As one of the atmosphere propagation delays, the tropospheric delay is a significant error source that should be properly handled in high-precision global navigation satellite system (GNSS) applications. We propose an improved zenith tropospheric delay (ZTD) modeling method whereby the piecewise model of the atmospheric refractivity is introduced. Compared with using the exponential model to fit ZTD in vertical direction, the ZTD piecewise model has a better performance. Based on ERA5 2.5° × 2.5° reanalysis data produced by the European Centre for Medium-Range Weather Forecasting (ECMWF) from 2013 to 2017, we establish the regional gridded ZTD model (RGZTD) using a trigonometric function for China and the surrounding areas, which ranges from 70° E to 135° E in longitude and from 15° N to 55° N in latitude. To verify the performance of RGZTD model, the ERA5 ZTD data in 2017–2018, the radiosonde ZTD data from 86 radiosonde stations over China in 2017–2018, and the tropospheric delay products on 251 GNSS stations from Crustal Movement Observation Network of China (CMONOC) in 2016–2017 are used as external compliance check data. The results show that the overall accuracy of RGZTD model is better than that of exponential model, UNB3m model, and GPT3 model. Moreover, the accuracy can be improved by about 13.4%, 7.1%, and 6.2% when ERA5 reanalysis data, radiosonde data, and CMONOC data are used as reference values, respectively. High-accuracy ZTD data can be provided because the RGZTD model takes into account the vertical variation of ZTD through the new piecewise model. Full article
(This article belongs to the Special Issue Satellite Observation for Atmospheric Modeling)
Show Figures

Graphical abstract

Graphical abstract
Full article ">Figure 1
<p>Geographic distribution of the 86 radiosonde stations.</p>
Full article ">Figure 2
<p>Geographic distribution of the 251 GNSS stations.</p>
Full article ">Figure 3
<p>Fitting residuals of the exponential model and the piecewise model at different grid points.</p>
Full article ">Figure 4
<p>Comparison of estimated parameters (Original data) and results of spectral analysis (Model) at the grid point (longitude 100° and latitude 30°) in 2013–2017.</p>
Full article ">Figure 5
<p>Distribution of bias and RMS of RGZTD model, Exponential model, GPT3 model and UNB3M model over China and the surrounding areas, where the ERA5 ZTD data is the reference value.</p>
Full article ">Figure 6
<p>Distribution of bias and RMS of RGZTD model, Exponential model, GPT3 model and UNB3M model in China, where the radiosonde ZTD data is the reference value.</p>
Full article ">Figure 7
<p>Distribution of bias and RMS of RGZTD model, Exponential model, GPT3 model and UNB3M model in China, where the CMONOC ZTD data is the reference value.</p>
Full article ">
17 pages, 5999 KiB  
Article
SHAtropE—A Regional Gridded ZTD Model for China and the Surrounding Areas
by Junping Chen, Jungang Wang, Ahao Wang, Junsheng Ding and Yize Zhang
Remote Sens. 2020, 12(1), 165; https://doi.org/10.3390/rs12010165 - 2 Jan 2020
Cited by 26 | Viewed by 2822
Abstract
A regional zenith tropospheric delay (ZTD) empirical model, referred to as SHAtropE (SHanghai Astronomical observatory tropospheric delay model—Extended), is developed and provides tropospheric propagation delay corrections for users in China and the surrounding areas with improved accuracy. The SHAtropE model was developed based [...] Read more.
A regional zenith tropospheric delay (ZTD) empirical model, referred to as SHAtropE (SHanghai Astronomical observatory tropospheric delay model—Extended), is developed and provides tropospheric propagation delay corrections for users in China and the surrounding areas with improved accuracy. The SHAtropE model was developed based on the ZTD time series of the continuous GNSS sites from the Crustal Movement Observation Network of China (CMONOC) and GNSS sites of surrounding areas. It combines the exponential and periodical functions and is provided as regional grids with a resolution of 2.5° × 2.0° in longitude and latitude. At each grid point, the exponential function converts the ZTD from the site height to the ellipsoid, and the periodical terms, including both annual and semi-annual periods, describe ZTD’s temporal variation. Moreover, SHAtropE also provides the predicted ZTD uncertainty, which is valuable in Precise Point Positioning (PPP) with ZTD being constrained for faster convergence. The data of 310 GNSS sites over 7 years were used to validate the new model. Results show that the SHAtropE ZTD has an accuracy of 3.5 cm in root mean square (RMS) quantity, which has a mean improvement of 35.2% and 5.4% over the UNB3m (5.4 cm) and GPT3 (3.7 cm) models, respectively. The predicted uncertainty of SHAtropE ZTD shows seasonal variations, where the values are larger in summer than in winter. By applying the SHAtropE model in the static PPP, the convergence time of GPS-only and BDS-only solutions are reduced by 8.1% and 14.5% respectively compared to the UNB3m model, and the reductions are 6.9% and 11.2% respectively for the GPT3 model. As no meteorological data are required for the implementation of the model, the SHAtropE could thus be a refined tropospheric model for GNSS users in mainland China and the surrounding areas. The method of modeling the ZTD uncertainty can also be used in further global tropospheric delay modeling. Full article
Show Figures

Graphical abstract

Graphical abstract
Full article ">Figure 1
<p>(<b>a</b>) Distribution of sites used and (<b>b</b>) the valid days of each site. The non-Crustal Movement Observation Network of China (CMONOC) site in panel (<b>a</b>) are marked with red edge, the color bar in (<b>a</b>) shows the site height in km.</p>
Full article ">Figure 2
<p>Parameters of the empirical temporal zenith tropospheric delay (ZTD) variations model of each site. (<b>a</b>) fitting root mean square (RMS); (<b>b</b>) the constant term <span class="html-italic">A</span><sub>0</sub>; (<b>c</b>) annual amplitude <span class="html-italic">A</span><sub>1</sub>; (<b>d</b>) initial phase of annual term <span class="html-italic">d</span><sub>1</sub>; (<b>e</b>) semi-annual amplitude <span class="html-italic">A</span><sub>2</sub>; (<b>f</b>) initial phase of semi-annual term <span class="html-italic">d</span><sub>2</sub>. It should be noted that the amplitudes are modified to make the phase terms continuous and in the range of (0, 90) and (−45, 45) for the annual and semi-annual terms, respectively.</p>
Full article ">Figure 3
<p>The fit parameters of the absolute ZTD fit residuals. (<b>a</b>) the ratio between the RMS of RAW ZTD fit residuals and the RMS of modeled residuals; (<b>b</b>) the constant term <span class="html-italic">B</span><sub>0</sub>; (<b>c</b>) annual amplitude <span class="html-italic">B</span><sub>1</sub>; (<b>d</b>) initial phase of annual term <span class="html-italic">f</span><sub>1</sub>; (<b>e</b>) semi-annual amplitude <span class="html-italic">B</span><sub>2</sub>; (<b>f</b>) initial phase of semi-annual term <span class="html-italic">f</span><sub>2</sub>.</p>
Full article ">Figure 4
<p>Annual average ZTD w.r.t. site ellipsoidal height and the exponential fitting curves. The scaled height and the fit RMS are also presented in the figure.</p>
Full article ">Figure 5
<p>(<b>a</b>) The constant term <span class="html-italic">A</span><sub>0</sub><sub>,<span class="html-italic">e</span></sub>, (<b>b</b>) the annual amplitude term <span class="html-italic">A</span><sub>1</sub><sub>,<span class="html-italic">e</span></sub>, and (<b>c</b>) the semi-annual term <span class="html-italic">A</span><sub>2</sub><sub>,<span class="html-italic">e</span></sub> of ZTD scaled on the ellipsoid of each site.</p>
Full article ">Figure 6
<p>RAW ZTD (green) and SHAtropE ZTD (red) for two sites: NMER (<b>left</b>) and YNLJ (<b>right</b>). The absolute value (magenta) of the differences between RAW ZTD and SHAtropE, and the predicted uncertainty provided by SHAtropE (black) are presented with an offset (2.05 m at NMER and 1.50 m at YNLJ) for better visualization.</p>
Full article ">Figure 7
<p>Comparisons between RAW ZTD and empirical models during the period of 2012–2018. Left: mean value of ZTD biases for (<b>a</b>) SHAtropE, (<b>c</b>) UNB3m, and (<b>e</b>) GPT3; Right: RMS values of the ZTD biases for (<b>b</b>) SHAtropE, (<b>d</b>) UNB3m, and (<b>f</b>) GPT3.</p>
Full article ">Figure 8
<p>Mean values (<b>left panel</b>) and RMS values (<b>right panel</b>) of the ZTD bias for the three different models: SHAtropE (red), UNB3m (green), and GPT3 (blue). The statistics of two periods: 2012–2017 and 2018 are presented separately, and the value of the whole period is presented in the legend.</p>
Full article ">Figure 9
<p>Left: predicted ZTD uncertainty of SHAtropE during the period of 2012–2018 in different seasons: (<b>a</b>) Mar-Apr-May, (<b>c</b>) Jun-Jul-Aug, (<b>e</b>) Sep-Oct-Nov, and (<b>g</b>) Dec-Jan-Feb; Right: the difference between predicted uncertainty of SHAtropE and the RMS value of SHAtropE ZTD w.r.t. RAW ZTD during the period of 2012–2018 for different seasons: (<b>b</b>) Mar-Apr-May, (<b>d</b>) Jun-Jul-Aug, (<b>f</b>) Sep-Oct-Nov, and (<b>h</b>) Dec-Jan-Feb.</p>
Full article ">Figure 10
<p>RMS statistics of the SHAtropE ZTD RMS w.r.t. RAW ZTD, and the predicted ZTD uncertainty of the model during 2012–2017 (red) and 2018 (blue) in different seasons: (<b>a</b>) Mar-Apr-May, (<b>b</b>) Jun-Jul-Aug, (<b>c</b>) Sep-Oct-Nov, and (<b>d</b>) Dec-Jan-Feb. The average values of the whole period 2012-2018 are presented in the legend.</p>
Full article ">Figure 11
<p>The improvement of average convergence time of static PPP with SHAtropE model for GPS-only and BDS-only solutions compared to UNB3m and GPT3 models. (<b>a</b>) UNB3m—SHAtropE for GPS-only PPP, (<b>b</b>) UNB3m—SHAtropE for BDS-only PPP, (<b>c</b>) GPT3—SHAtropE for GPS-only PPP, (<b>d</b>) GPT3—SHAtropE for BDS-only PPP.</p>
Full article ">Figure 12
<p>Average convergence time of static PPP with three different tropospheric models (SHAtropE (red), UNB3m (green), and GPT3 (blue)) for the GPS-only and BDS-only solutions.</p>
Full article ">
4047 KiB  
Article
SSIEGNOS: A New Asian Single Site Tropospheric Correction Model
by Liangke Huang, Shaofeng Xie, Lilong Liu, Junyu Li, Jun Chen and Chuanli Kang
ISPRS Int. J. Geo-Inf. 2017, 6(1), 20; https://doi.org/10.3390/ijgi6010020 - 17 Jan 2017
Cited by 8 | Viewed by 5049
Abstract
This paper proposes a new Asian single site tropospheric correction model called the Single Site Improved European Geostationary Navigation Overlay Service model (SSIEGNOS) by refining the European Geostationary Navigation Overlay Service (EGNOS) model at a single site. The performance of the SSIEGNOS model [...] Read more.
This paper proposes a new Asian single site tropospheric correction model called the Single Site Improved European Geostationary Navigation Overlay Service model (SSIEGNOS) by refining the European Geostationary Navigation Overlay Service (EGNOS) model at a single site. The performance of the SSIEGNOS model is analyzed. The results show that (1) the bias and root mean square (RMS) error of zenith tropospheric delay (ZTD) calculated from the EGNOS model are 0.12 cm and 5.87 cm, respectively; whereas those of the SSIEGNOS model are 0 cm and 2.52 cm, respectively. (2) The bias and RMS error show seasonal variation in the EGNOS model; however, little seasonal variation is observed in the SSIEGNOS model. (3) The RMS error decreases with increasing altitude or latitude in the two models; however, no such relationships were found in the bias. In addition, the annual predicted bias and RMS error in Asia are −0.08 cm and 3.14 cm for the SSIEGNOS model, respectively; however, the EGNOS and UNB3m (University of New Brunswick) models show comparable predicted results. Relative to the EGNOS model, the annual predicted bias and RMS error decreased by 55% and 48%, respectively, for the SSIEGNOS model. Full article
(This article belongs to the Special Issue Recent Advances in Geodesy & Its Applications)
Show Figures

Figure 1

Figure 1
<p>Distribution of the IGS sites in Asia. The abscissa represents longitude, and the ordinate represents latitude.</p>
Full article ">Figure 2
<p>Variation of the daily bias and spectral analysis based on Fourier transformation at IISC, LHAZ, WUHN, GMSD, POL2 and NOVM sites in 2008–2010. The latitude, longitude, and altitude of each site are listed in the brackets.</p>
Full article ">Figure 3
<p>Variation of the daily bias and RMS in 2008–2010 at sites IRKJ, CHUM, TSK2, and CUSV for the EGNOS and SSIEGNOS models. The black line represents EGNOS model and the red line represents SSIEGNOS model.</p>
Full article ">Figure 4
<p>Variation of the monthly bias and RMS error in 2008–2010 over Asia. Yellow bars and red bars indicate the bias and RMS error of the EGNOS model and SSIEGNOS model, respectively.</p>
Full article ">Figure 5
<p>Distribution of annual bias and RMS error of the EGNOS and SSIEGNOS models from 2008–2010 over Asia. The color denotes the magnitude of the annual bias and RMS error.</p>
Full article ">Figure 6
<p>(<b>a</b>,<b>b</b>) show the annual bias and RMS error in each altitude range, respectively; (<b>c</b>,<b>d</b>) denote the correlations between altitude and bias and RMS error, respectively. Black stems and white bars represent the mean bias and RMS error of the EGNOS and SSIEGNOS models, respectively.</p>
Full article ">Figure 7
<p>(<b>a</b>,<b>b</b>) show the annual bias and RMS error in each latitude range; (<b>c</b>,<b>d</b>) show the correlations between bias and latitude, respectively. Black stems and white bars denote the mean bias and RMS error of the EGNOS and SSIEGNOS models, respectively.</p>
Full article ">Figure 8
<p>(<b>a</b>,<b>b</b>) show the annual bias and RMS error in each longitude range; whereas (<b>c</b>,<b>d</b>) show the mean correlations between bias and longitude. Black stems and white bars represent the mean bias and RMS error of the EGNOS and SSIEGNOS models, respectively.</p>
Full article ">Figure 9
<p>The distribution of the annual predicted bias and RMS error of the EGNOS, UNB3m, and SSIEGNOS models over Asia in 2011. The color denotes the magnitudes of the annual predicted bias and RMS error.</p>
Full article ">Figure 10
<p>Distribution histogram of predicted bias and RMS error of the EGNOS, UNB3m, and SSIEGNOS models over Asia in 2011. The left shows the EGNOS model results, the middle shows the UNB3m model results, and the right shows the SSIEGNOS model results. The vertical axis denotes the number of samples.</p>
Full article ">Figure 11
<p>(<b>a</b>,<b>b</b>) and (<b>c</b>,<b>d</b>) show the monthly and seasonal variations of predicted bias and RMS error in 2011 over Asia using the EGNOS, UNB3m, and SSIEGNOS models, respectively. The blue color denotes the EGNOS model, the green color denotes the UNB3m model, and the red color denotes the SSIEGNOS model.</p>
Full article ">Figure 12
<p>(<b>a</b>,<b>b</b>) Time series of daily predicted bias and RMS from 2011–2012 at the IRKT site. The blue line denotes the EGNOS model, the green line denotes the UNB3m model, and the red line denotes the SSIEGNOS model. (<b>c</b>–<b>h</b>) Histograms of the daily predicted bias and RMS error from 2011–2012 for the three models, respectively.</p>
Full article ">Figure 13
<p>(<b>a</b>,<b>b</b>) Time series of daily predicted bias and RMS error from 2011–2012 at the PIMO site. The blue line denotes the EGNOS model, the green line denotes the UNB3m model, and the red line denotes the SSIEGNOS model. (<b>c</b>–<b>h</b>) Histograms of the daily predicted bias and RMS error from 2011–2012 for the three models.</p>
Full article ">Figure 14
<p>(<b>a</b>,<b>b</b>) Time series of daily predicted bias and RMS error from 2011–2012 at the POL2 site. The blue line denotes the EGNOS model, the green line denotes the UNB3m model, and the red line denotes the SSIEGNOS model. (<b>c</b>–<b>h</b>) Histograms of the daily predicted bias and RMS error from 2011–2012 for the three models.</p>
Full article ">Figure 15
<p>(<b>a</b>,<b>b</b>) Time series of daily predicted bias and RMS error from 2011–2012 at the TSK2 site. The blue line denotes the EGNOS model, the green line denotes the UNB3m model, and the red line denotes the SSIEGNOS model. (<b>c</b>–<b>h</b>) Histograms of the daily predicted bias and RMS error from 2011–2012 for the three models.</p>
Full article ">Figure 16
<p>Monthly mean predicted bias and RMS from 2011–2012 at the TSK2, POL2, IRKT, and TSK2 sites. The blue bars, green bars, and red bars denote the monthly bias and RMS error of the EGNOS, UNB3m, and SSIEGNOS models, respectively.</p>
Full article ">Figure 17
<p>Seasonal mean predicted bias and RMS error from 2011–2012 at the TSK2, POL2, IRKT, and TSK2 sites. The blue bars, green bars and red bars denote the monthly bias and RMS error of the EGNOS, UNB3m, and SSIEGNOS models, respectively.</p>
Full article ">
4066 KiB  
Article
Assessment of Three Tropospheric Delay Models (IGGtrop, EGNOS and UNB3m) Based on Precise Point Positioning in the Chinese Region
by Hongxing Zhang, Yunbin Yuan, Wei Li, Ying Li and Yanju Chai
Sensors 2016, 16(1), 122; https://doi.org/10.3390/s16010122 - 20 Jan 2016
Cited by 31 | Viewed by 6059
Abstract
Tropospheric delays are one of the main sources of errors in the Global Navigation Satellite System (GNSS). They are usually corrected by using tropospheric delay models, which makes the accuracy of the models rather critical for accurate positioning. To provide references for suitable [...] Read more.
Tropospheric delays are one of the main sources of errors in the Global Navigation Satellite System (GNSS). They are usually corrected by using tropospheric delay models, which makes the accuracy of the models rather critical for accurate positioning. To provide references for suitable models to be chosen for GNSS users in China, we conduct herein a comprehensive study of the performances of the IGGtrop, EGNOS and UNB3m models in China. Firstly, we assess the models using 5 years’ Global Positioning System (GPS) derived Zenith Tropospheric Delay (ZTD) series from 25 stations of the Crustal Movement Observation Network of China (CMONOC). Then we study the effects of the models on satellite positioning by using various Precise Point Positioning (PPP) cases with different tropospheric delay resolutions, the observation data processed in PPP is from 21 base stations of CMONOC for a whole year of 2012. The results show that: (1) the Root Mean Square (RMS) of the IGGtrop model is about 4.4 cm, which improves the accuracy of ZTD estimations by about 24% for EGNOS and 19% for UNB3m; (2) The positioning error in the vertical component of the PPP solution obtained by using the IGGtrop model is about 15.0 cm, which is about 30% and 21% smaller than those of the EGNOS and UNB3m models, respectively. In summary, the IGGtrop model achieves the best performance among the three models in the Chinese region. Full article
(This article belongs to the Section Remote Sensors)
Show Figures

Figure 1

Figure 1
<p>Distribution of 25 selected stations of CMONOC used in this study.</p>
Full article ">Figure 2
<p>Time series of ZTD derived from GPS and three empirical models (IGGtrop, EGNOS and UNB3m) over the time period from 2009 to 2013.</p>
Full article ">Figure 3
<p>Histogram of the biases for the IGGtrop, EGNOS and UNB3m models over the period from 2009 to 2013 at four exemplary stations of JIXN, BJFS, HRBN and ZHNZ.</p>
Full article ">Figure 4
<p>Temporal variations of monthly mean RMS (<b>a</b>) and Bias (<b>b</b>) for the IGGtrop, EGNOS and UNB3m models at four exemplary stations of BJFS, ZHNZ, KMIN and SHAO.</p>
Full article ">Figure 5
<p>Mean bias (<b>a</b>) and RMS (<b>b</b>) over the period from 2009 to 2013 for the IGGtrop, EGNOS and UNB3m models. Stations are listed from left to right of the x-axis according to their station height from low to high.</p>
Full article ">Figure 6
<p>Positioning errors of the conventional PPP and three model-based PPP (IGGtrop-based, EGNOS-based, UNB3m-based) at stations of BJFS, HRBN, KMIN and LHAZ, and the epoch interval is 30 s, the DOY are 28 (<b>a</b>) and 200 (<b>b</b>) in 2012.</p>
Full article ">Figure 7
<p>Mean positioning errors of the conventional PPP, IGGtrop-based, EGNOS-based and UNB3m-based PPP solutions over the period from January to December 2012 at selected stations. The upper, medium and bottom panels show the positioning errors in north, east and up directions, respectively.</p>
Full article ">Figure 8
<p>Time series of positioning errors for the conventional, IGGtrop-based, EGNOS-based and UNB3m-based PPP solutions at stations of BJFS, ZHNZ, XIAG and LHAZ, the DOY represents the day of year in 2012.</p>
Full article ">
Back to TopTop