Jufeng Yang, Shuhui Li, Aochuan Zhang, Shaoqiu Chen, Han Wang
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引用次数: 0
Abstract
This paper aims to compare the performance of the low-cost Global Navigation Satellite System (GNSS) receiver u-blox ZED-F9P and the geodetic receiver JAVAD SIGMA G3T on vertical total electron content (VTEC) estimation, and to evaluate the impacts of different antennas on VTEC estimation. Using the undifferenced and uncombined Precise Point Positioning (PPP) algorithm to process GNSS data on April 15, September 11, and September 12, 2021. Then we compared the accuracy of VTEC and differential code bias (DCB) estimation between the low-cost GNSS receiver and the geodetic receiver. The results showed that VTEC extracted from low-cost GNSS receiver and geodetic receiver are consistent with the Global Ionospheric Model (GIM) products. However, the low-cost GNSS receiver’s VTEC accuracy is slightly lower, with the residual root mean square (RMS) values ranging from 1.07 to 1.72 TECU (Total Electron Content Unit) and the absolute mean bias ranging from −1.48 to −0.85 TECU. Additionally, satellite DCBs from the geodetic receiver were closer to CAS products than those from the low-cost GNSS receiver, with more satellites exhibiting absolute bias less than 1 nanosecond. Moreover, we analyzed the impact of different antennas (SEPCHOKE_B3E6 and JAVAD GrAnt-G3T) on VTEC estimation. For two receivers, VTEC differences between antennas are less than 1 TECU, with RMS of the biases between different antennas less than 0.35 TECU and mean biases do not exceed 0.21 TECU.
期刊介绍:
Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered.
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