High-precision VTEC derivation with GEONET
Creators
- 1. University of Chinese Academy of Sciences (China)
- 2. National Astronomical Observatories, Chinese Academy of Sciences (China)
- 3. National Institute of Information and Communications Technology (Japan)
Description
This paper proposes a new technique, namely Phase bias-based Small Grid Model (PSGM), to derive absolute ionospheric vertical total electron content (VTEC) with observations of Global Navigation Satellite System Earth Observation Network of Japan (GEONET). The proposed technique deals with the phase observations alone without handling the pseudoranges, which reduces the noise in VTEC estimation. A new parameter, the arc bias (Barc), is introduced to combine the phase ambiguities and differential phase biases. To solve Barc, equations are constructed under the assumption that the VTEC is identical in the same 0.1° × 0.1° grid. The performance of PSGM is evaluated with the observations in solar maximum year 2014. The root mean square error (RMSE) of PSGM is 0.40 TECU in average, the maximum RMSE is 0.73 TECU and the minimum RMSE is 0.26 TECU. The fitting accuracy of the VTEC results is improved compared with most of the existing methods.
Additional details
Identifiers
Publishing Information
- Journal Title
- Earth, Planets and Space (Online)
- Journal Volume
- 72
- Journal Issue
- 1
- Journal Page Range
- vp.
- ISSN
- 1880-5981
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 55062759
- Subject category
- S97: MATHEMATICAL METHODS AND COMPUTING; S58: GEOSCIENCES;
- Descriptors DEI
- ACCURACY; COMPARATIVE EVALUATIONS; DIFFERENTIAL EQUATIONS; ELECTRONS; ERRORS; GRIDS; NOISE; PERFORMANCE; SATELLITES; SOLAR RADIATION; TIME-SERIES ANALYSIS
- Descriptors DEC
- ELECTRODES; ELEMENTARY PARTICLES; EQUATIONS; EVALUATION; FERMIONS; LEPTONS; MATHEMATICS; RADIATIONS; STATISTICS; STELLAR RADIATION
Optional Information
- Copyright
- Copyright (c) 2020 © The Author(s) 2020