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handle: 10261/295631 , 2117/385245
AbstractIonospheric delay modeling is not only important for Global Navigation Satellite System (GNSS) based space weather study and monitoring, but also an efficient tool to speed up the convergence time of Precise Point Positioning (PPP). In this study, a novel model, denoted as Quasi-4-Dimension Ionospheric Modeling (Q4DIM) is proposed for wide-area high precision ionospheric delay correction. In Q4DIM, the Line Of Sight (LOS) ionospheric delays from a GNSS station network are divided into different clusters according to not only the location of latitude and longitude, but also satellite elevation and azimuth. Both Global Ionosphere Map (GIM) and Slant Ionospheric Delay (SID) models that are traditionally used for wide-area and regional ionospheric delay modeling, respectively, can be regarded as the special cases of Q4DIM by defining proper grids in latitude, longitude, elevation, and azimuth. Thus, Q4DIM presents a resilient model that is capable for both wide-area coverage and high precision. Four different sets of clusters are defined to illustrate the properties of Q4DIM based on 200 EUREF Permanent Network (EPN) stations. The results indicate that Q4DIM is compatible with the GIM products. Moreover, it is proved that by inducting the elevation and azimuth angle dependent residuals, the precision of the 2-dimensional GIM-like model, i.e., Q4DIM 2-Dimensional (Q4DIM-2D), is improved from around 1.5 Total Electron Content Units (TECU) to better than 0.5 TECU. In addition, treating Q4DIM as a 4-dimensional matrix in latitude, longitude, elevation, and azimuth, whose sparsity is less than 5%, can result in its feasibility in a bandwidth-sensitive applications, e.g., satellite-based Precising Point Positioning Real-Time Kinematic (PPP-RTK) service. Finally, the advantages of Q4DIM in PPP over the 2-dimensional models are demonstrated with the one month's data from 30 EPN stations in both high solar activity year 2014 and low solar activity year 2020.
Classificació AMS::90 Operations research, Programming (Mathematics), Design, Classificació AMS::85 Astronomy and astrophysics, PPP, Wide‑area, mathematical programming::90C Mathematical programming, Física matemàtica, Classificació AMS::90 Operations research, mathematical programming::90C Mathematical programming, Undifferenced and uncombined observation, Ionosphere delay modeling, DESIGN, Àrees temàtiques de la UPC::Matemàtiques i estadística::Matemàtica aplicada a les ciències, Astronomy and astrophysics, Programació (Matemàtica), T1-995, Àrees temàtiques de la UPC::Matemàtiques i estadística::Investigació operativa::Programació matemàtica, Technology (General), Wide-area
Classificació AMS::90 Operations research, Programming (Mathematics), Design, Classificació AMS::85 Astronomy and astrophysics, PPP, Wide‑area, mathematical programming::90C Mathematical programming, Física matemàtica, Classificació AMS::90 Operations research, mathematical programming::90C Mathematical programming, Undifferenced and uncombined observation, Ionosphere delay modeling, DESIGN, Àrees temàtiques de la UPC::Matemàtiques i estadística::Matemàtica aplicada a les ciències, Astronomy and astrophysics, Programació (Matemàtica), T1-995, Àrees temàtiques de la UPC::Matemàtiques i estadística::Investigació operativa::Programació matemàtica, Technology (General), Wide-area
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