Global Ionosphere Mapping and Differential Code Bias Estimation during Low and High Solar Activity Periods with GIMAS Software

被引:37
|
作者
Zhang, Qiang [1 ]
Zhao, Qile [1 ,2 ]
机构
[1] Wuhan Univ, GNSS Res Ctr, 129 Luoyu Rd, Wuhan 430079, Hubei, Peoples R China
[2] Wuhan Univ, Collaborat Innovat Ctr Earth & Space Sci, 129 Luoyu Rd, Wuhan 430079, Hubei, Peoples R China
基金
中国国家自然科学基金;
关键词
global ionosphere mapping; total electron content; differential code bias; GNSS; Jason-2; spherical harmonic expansion; GIMAS; TOTAL ELECTRON-CONTENT; POSITIONING SYSTEM; VTEC; SERVICE; MAPS;
D O I
10.3390/rs10050705
中图分类号
X [环境科学、安全科学];
学科分类号
08 ; 0830 ;
摘要
Ionosphere research using the Global Navigation Satellite Systems (GNSS) techniques is a hot topic, with their unprecedented high temporal and spatial sampling rate. We introduced a new GNSS Ionosphere Monitoring and Analysis Software (GIMAS) in order to model the global ionosphere vertical total electron content (VTEC) maps and to estimate the GPS and GLObalnaya NAvigatsionnaya Sputnikovaya Sistema (GLONASS) satellite and receiver differential code biases (DCBs). The GIMAS-based Global Ionosphere Map (GIM) products during low (day of year from 202 to 231, in 2008) and high (day of year from 050 to 079, in 2014) solar activity periods were investigated and assessed. The results showed that the biases of the GIMAS-based VTEC maps relative to the International GNSS Service (IGS) Ionosphere Associate Analysis Centers (IAACs) VTEC maps ranged from -3.0 to 1.0 TECU (TEC unit) (1 TECU = 1 x 10(16) electrons/m(2)). The standard deviations (STDs) ranged from 0.7 to 1.9 TECU in 2008, and from 2.0 to 8.0 TECU in 2014. The STDs at a low latitude were significantly larger than those at middle and high latitudes, as a result of the ionospheric latitudinal gradients. When compared with the Jason-2 VTEC measurements, the GIMAS-based VTEC maps showed a negative systematic bias of about -1.8 TECU in 2008, and a positive systematic bias of about +2.2 TECU in 2014. The STDs were about 2.0 TECU in 2008, and ranged from 2.2 to 8.5 TECU in 2014. Furthermore, the aforementioned characteristics were strongly related to the conditions of the ionosphere variation and the geographic latitude. The GPS and GLONASS satellite and receiver P1-P2 DCBs were compared with the IAACs DCBs. The root mean squares (RMSs) were 0.16-0.20 ns in 2008 and 0.13-0.25 ns in 2014 for the GPS satellites and 0.26-0.31 ns in 2014 for the GLONASS satellites. The RMSs of receiver DCBs were 0.21-0.42 ns in 2008 and 0.33-1.47 ns in 2014 for GPS and 0.67-0.96 ns in 2014 for GLONASS. The monthly stability of the GPS satellite DCBs was about 0.04 ns (0.07 ns) in 2008 (2014) and that for the GLONASS satellite DCBs was about 0.09 ns in 2014. The receiver DCBs were less stable than the satellite DCBs, with a mean value of about 0.16 ns (0.47 ns) in 2008 (2014) for GPS, and 0.48 ns in 2014 for GLONASS. It can be demonstrated that the GIMAS software had a high accuracy and reliability for the global ionosphere monitoring and analysis.
引用
收藏
页数:23
相关论文
共 27 条
  • [21] Ionosphere Total Electron Content Modeling and Multi-Type Differential Code Bias Estimation Using Multi-Mode and Multi-Frequency Global Navigation Satellite System Observations
    Wang, Qisheng
    Zhu, Jiaru
    Hu, Feng
    REMOTE SENSING, 2023, 15 (18)
  • [22] Observations of GW/TID oscillations in the F2 layer at low latitude during high and low solar activity, geomagnetic quiet and disturbed periods
    Klausner, V.
    Fagundes, P. R.
    Sahai, Y.
    Wrasse, C. M.
    Pillat, V. G.
    Becker-Guedes, F.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2009, 114
  • [23] Impact of temporal resolution in global ionospheric models on satellite positioning during low and high solar activity years of solar cycle 24
    Abdelaziz, Ahmed
    Zhang, Xiaohong
    Ren, Xiaodong
    Rabah, Mostafa
    Sedeek, Ahmed
    JOURNAL OF APPLIED GEODESY, 2024,
  • [24] Assessment of the Ionospheric and Tropospheric Effects in Location Errors of Data Collection Platforms in Equatorial Region during High and Low Solar Activity Periods
    da Silva, Aurea Aparecida
    Yamaguti, Wilson
    Kuga, Helio Koiti
    Celestino, Claudia Celeste
    MATHEMATICAL PROBLEMS IN ENGINEERING, 2012, 2012
  • [25] High and mid latitude and near subsolar point ionospheric and thermospheric responses to the solar flares and geomagnetic storms during low solar activity periods of 2017 and 2020
    Sur, Dibyendu
    Ray, Sarbani
    Paul, Ashik
    ADVANCES IN SPACE RESEARCH, 2022, 70 (01) : 157 - 178
  • [26] Assimilating Space-Based Thermospheric Neutral Density (TND) Data Into the TIE-GCM Coupled Model During Periods With Low and High Solar Activity
    Kosary, Mona
    Farzaneh, Saeed
    Schumacher, Maike
    Forootan, Ehsan
    SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS, 2024, 22 (04):
  • [27] The combined effects of electrojet strength and the geomagnetic activity (Kp-index) on the post sunset height rise of the F-layer and its role in the generation of ESF during high and low solar activity periods
    Ram, S. Tulasi
    Rao, P. V. S. Rama
    Prasad, D. S. V. V. D.
    Niranjan, K.
    Babu, A. Raja
    Sridharan, R.
    Devasia, C. V.
    Ravindran, Sudha
    ANNALES GEOPHYSICAE, 2007, 25 (09) : 2007 - 2017