Articles | Volume 41, issue 2
https://doi.org/10.5194/angeo-41-465-2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/angeo-41-465-2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Estimation and evaluation of hourly Meteorological Operational (MetOp) satellites' GPS receiver differential code biases (DCBs) with two different methods
Linlin Li
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China
School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing, 100049, China
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China
School of Surveying and Land Information Engineering, Henan Polytechnic University, Jiaozuo, 454003, China
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Yuanyuan Zhang, Ning Wang, and Shuanggen Jin
EGUsphere, https://doi.org/10.5194/egusphere-2025-992, https://doi.org/10.5194/egusphere-2025-992, 2025
This preprint is open for discussion and under review for Atmospheric Measurement Techniques (AMT).
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Satellite remote sensing helps monitor dust storms in East Asia, but its effectiveness is still limited. Our study compared five satellite products that use ground-based PM10 data. Most products agreed on the daily dust distribution, with AAI performing best under cloud cover. MODIS AOD performed best, followed by Himawari-8 AOD. This study improves dust and sparseness monitoring in East Asia.
Mohamed Darrag, Shuanggen Jin, Andrés Calabia, and Aalaa Samy
Ann. Geophys., 40, 359–377, https://doi.org/10.5194/angeo-40-359-2022, https://doi.org/10.5194/angeo-40-359-2022, 2022
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We investigated the possible widening of the tropical belt along with the probable drivers and impacts based on high-accuracy, high-resolution GNSS RO data (2001–2020). The results show that the tropical belt has significant expansion in the Northern Hemisphere, while the Southern Hemisphere has no significant expansion.
W. Geng, W. Zhou, and S. Jin
Int. Arch. Photogramm. Remote Sens. Spatial Inf. Sci., XLIV-M-3-2021, 63–66, https://doi.org/10.5194/isprs-archives-XLIV-M-3-2021-63-2021, https://doi.org/10.5194/isprs-archives-XLIV-M-3-2021-63-2021, 2021
Qisheng Wang, Shuanggen Jin, and Youjian Hu
Ann. Geophys., 38, 1115–1122, https://doi.org/10.5194/angeo-38-1115-2020, https://doi.org/10.5194/angeo-38-1115-2020, 2020
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In this paper, the receiver differential code bias (DCB) of BDS (BeiDou Navigation Satellite System) is estimated as the changing parameter within 1 d with epoch-by-epoch estimates. The intraday variability of receiver DCB is analyzed from 30 d of Multi-GNSS Experiment observations. In particular, the intraday stability of receiver DCB for the BDS-3 and BDS-2 observations is compared. The result shows that the intraday stability of BDS-3 receiver DCB is better than that of BDS-2 receiver DCB.
Andres Calabia and Shuanggen Jin
Ann. Geophys., 37, 989–1003, https://doi.org/10.5194/angeo-37-989-2019, https://doi.org/10.5194/angeo-37-989-2019, 2019
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Atmospheric drag due to mass density distribution, particularly during storm-time, is of great importance for low Earth orbit precise orbit determination, and for the understanding of magnetosphere–ionosphere–thermosphere phenomena. In this paper, we investigate solar cycle, seasonal, and hemispheric asymmetry dependencies of thermospheric mass density disturbances due to magnetospheric forcing, from 10-year (2003–2013) continuous time series of GRACE estimates.
Ming Shangguan, Wuke Wang, and Shuanggen Jin
Atmos. Chem. Phys., 19, 6659–6679, https://doi.org/10.5194/acp-19-6659-2019, https://doi.org/10.5194/acp-19-6659-2019, 2019
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A significant warming in the troposphere and cooling in the stratosphere are found in satellite measurements (2002–2017). The newest ERA5 data are first used for analyzing temperature and ozone trends in the UTLS and show the best quality compared to other reanalyses. According to model simulations, the temperature increase in the troposphere and ozone decrease in the NH stratosphere are mainly connected to a surface warming of the ocean and subsequent changes in atmospheric circulation.
N. B. Avsar, S. Jin, and S. H. Kutoglu
Int. Arch. Photogramm. Remote Sens. Spatial Inf. Sci., XLII-3-W4, 83–85, https://doi.org/10.5194/isprs-archives-XLII-3-W4-83-2018, https://doi.org/10.5194/isprs-archives-XLII-3-W4-83-2018, 2018
G. Gurbuz and S. Jin
Int. Arch. Photogramm. Remote Sens. Spatial Inf. Sci., XLII-3-W4, 239–243, https://doi.org/10.5194/isprs-archives-XLII-3-W4-239-2018, https://doi.org/10.5194/isprs-archives-XLII-3-W4-239-2018, 2018
Junhai Li and Shuanggen Jin
Ann. Geophys., 35, 403–411, https://doi.org/10.5194/angeo-35-403-2017, https://doi.org/10.5194/angeo-35-403-2017, 2017
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In this paper, we discuss the higher-order ionospheric effects on electron density estimation. We estimate the higher-order ionospheric effect carefully and obtain some conclusions. The results show that the second-order ionospheric effects cannot be ignored in precise ionospheric electron density estimation. The azimuth, the solar activity, and the occultation time and position are the main effect factors of the high-order ionospheric delay which we should consider.
S. G. Jin, R. Jin, and D. Li
Ann. Geophys., 34, 259–269, https://doi.org/10.5194/angeo-34-259-2016, https://doi.org/10.5194/angeo-34-259-2016, 2016
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The differential code bias (DCB) is one of main errors for high-precision GNSS TEC estimation and positioning applications. In this paper, daily DCBs of the BeiDou System (BDS) are estimated and investigated from multi-GNSS network observations (2013–2014), which are compared with GPS results. The DCB of BDS satellites is a little less stable than GPS results, especially for GEO satellites. Zero-mean condition effects are not the dominant factor for the higher RMS of BDS satellite DCB.
Related subject area
Subject: Earth's ionosphere & aeronomy | Keywords: Instruments and techniques
Comparison of meteor radar and satellite winds in the Brazilian equatorial region
Simulation of interferometric imaging with EISCAT_3D for fine-scale in-beam incoherent scatter spectra measurements
A technique for volumetric incoherent scatter radar analysis
Sounding of sporadic E layers from China Seismo-Electromagnetic Satellite (CSES) radio occultation and comparing with ionosonde measurements
Observing electric field and neutral wind with EISCAT 3D
Inferring thermospheric composition from ionogram profiles: a calibration with the TIMED spacecraft
Radar imaging with EISCAT 3D
Auroral ionospheric E region parameters obtained from satellite- based far-ultraviolet and ground-based ionosonde observations – effects of proton precipitation
Estimating satellite and receiver differential code bias using a relative Global Positioning System network
Validation of Clyde River SuperDARN radar velocity measurements with the RISR-C incoherent scatter radar
Ana Roberta Paulino, Delis Otildes Rodrigues, Igo Paulino, Lourivaldo Mota Lima, Ricardo Arlen Buriti, Paulo Prado Batista, Aaron Ridley, and Chen Wu
Ann. Geophys., 43, 183–191, https://doi.org/10.5194/angeo-43-183-2025, https://doi.org/10.5194/angeo-43-183-2025, 2025
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Comparisons of wind measurements using two different techniques (ground-based radar and satellite) in Brazil during 2006 were made in order to point out the advantages of each instrument for studies in the mesosphere and upper thermosphere. (i) For short-period variations, the measurements of the satellite were more advantageous. (ii) The monthly climatology using the radar was more appropriate. (iii) For long periods (longer than a few months), both instruments responded satisfactorily.
Devin Huyghebaert, Björn Gustavsson, Juha Vierinen, Andreas Kvammen, Matthew Zettergren, John Swoboda, Ilkka Virtanen, Spencer M. Hatch, and Karl M. Laundal
Ann. Geophys., 43, 99–113, https://doi.org/10.5194/angeo-43-99-2025, https://doi.org/10.5194/angeo-43-99-2025, 2025
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The EISCAT_3D radar is a new ionospheric radar under construction in the Fennoscandia region. The radar will make measurements of plasma characteristics at altitudes above approximately 60 km. The capability of the system to make these measurements at spatial scales of less than 100 m using multiple digitised signals from each of the radar antenna panels is highlighted. There are many ionospheric small-scale processes that will be further resolved using the techniques discussed here.
Johann Stamm, Juha Vierinen, Björn Gustavsson, and Andres Spicher
Ann. Geophys., 41, 55–67, https://doi.org/10.5194/angeo-41-55-2023, https://doi.org/10.5194/angeo-41-55-2023, 2023
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The study of some ionospheric events benefit from the knowledge of how the physics varies over a volume and over time. Examples are studies of aurora or energy deposition. With EISCAT3D, measurements of ion velocity vectors in a volume will be possible for the first time. We present a technique that uses a set of such measurements to estimate electric field and neutral wind. The technique relies on adding restrictions to the estimates. We successfully consider restrictions based on physics.
Chengkun Gan, Jiayu Hu, Xiaomin Luo, Chao Xiong, and Shengfeng Gu
Ann. Geophys., 40, 463–474, https://doi.org/10.5194/angeo-40-463-2022, https://doi.org/10.5194/angeo-40-463-2022, 2022
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We develop a new criterion to determine Es, i.e., when the mean value of the absolute value of the difference between the normalized SNR is greater than 3 times the standard deviation. We show that Es have strong seasonal variations, with the highest occurrence rates in the summer season at midlatitudes mainly located at 90–110 km at 14:00–20:00 LT. The comparison of Es altitudes from radio occultation profiles with ionosonde revealed a large correspondence between both measurement techniques.
Johann Stamm, Juha Vierinen, and Björn Gustavsson
Ann. Geophys., 39, 961–974, https://doi.org/10.5194/angeo-39-961-2021, https://doi.org/10.5194/angeo-39-961-2021, 2021
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Measurements of the electric field and neutral wind in the ionosphere are important for understanding energy flows or electric currents. With incoherent scatter radars (ISRs), we can measure the velocity of the ions, which depends on both the electrical field and the neutral wind. In this paper, we investigate methods to use ISR data to find reasonable values for both parameters. We find that electric field can be well measured down to 125 km height and neutral wind below this height.
Christopher J. Scott, Shannon Jones, and Luke A. Barnard
Ann. Geophys., 39, 309–319, https://doi.org/10.5194/angeo-39-309-2021, https://doi.org/10.5194/angeo-39-309-2021, 2021
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The composition of the upper atmosphere has been difficult to measure with localised observations relying on spacecraft, suborbital rockets or measurements of airglow from ground-based observatories. The height profile of ionisation within the neutral upper atmosphere is influenced by the composition of the neutral gas. We present a method for determining the neutral upper-atmosphere composition from measurements of the ionisation profile and compare these with spacecraft measurements.
Johann Stamm, Juha Vierinen, Juan M. Urco, Björn Gustavsson, and Jorge L. Chau
Ann. Geophys., 39, 119–134, https://doi.org/10.5194/angeo-39-119-2021, https://doi.org/10.5194/angeo-39-119-2021, 2021
Harold K. Knight
Ann. Geophys., 39, 105–118, https://doi.org/10.5194/angeo-39-105-2021, https://doi.org/10.5194/angeo-39-105-2021, 2021
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Comparisons were made of ground-based ionosonde (a type of radar) observations of the ionosphere and satellite-based observations of auroral far-ultraviolet emissions to determine whether a remote sensing algorithm for determining auroral ionospheric electron densities from far-ultraviolet emissions was biased by the presence of proton precipitation, and it was found that there was no such bias.
Alaa A. Elghazouly, Mohamed I. Doma, and Ahmed A. Sedeek
Ann. Geophys., 37, 1039–1047, https://doi.org/10.5194/angeo-37-1039-2019, https://doi.org/10.5194/angeo-37-1039-2019, 2019
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Receiver and satellite differential code biases (DCBs) are one of the main error sources in estimating precise global ionosphere maps (GIMs) from Global Positioning System (GPS) data. This paper introduces a mathematical model for estimating satellite and receiver DCBs from a GPS network written in the MATLAB environment. Our code was tested and compared with Ionosphere Associated Analysis Centers (IAAC) and other researchers' code results. The results show an improvement for estimated DCBs.
Alexander Koustov, Robert Gillies, and Peter Bankole
Ann. Geophys., 36, 1657–1666, https://doi.org/10.5194/angeo-36-1657-2018, https://doi.org/10.5194/angeo-36-1657-2018, 2018
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Clyde River (CLY) SuperDARN radar velocities reflecting plasma flows in the ionosphere are consistent with measurements by the incoherent scatter radar RISR. While agreement is good in the range of RISR velocity magnitudes of 0–700 m s−1, CLY velocities become progressively smaller at faster flows. In one example of strong disagreements between the instruments, by 200 m s−1, the radars monitored strongly sheared flows. Validation of the CLY radar confirms the reliability of SuperDARN operation.
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Short summary
We used the spherical harmonic function (SHF) and the local spherical symmetry (LSS) assumption methods to calculate the hourly and daily LEO satellite GPS differential code bias (DCB). The SHF method is more stable and precise than the LSS assumption. The daily DCB estimation is more accurate and stable than the hourly DCB due to more observation data. Hourly DCBs have large changes in one day, mainly be attributed to random errors because these error time series have a normal distribution.
We used the spherical harmonic function (SHF) and the local spherical symmetry (LSS) assumption...