From: Status of CAS global ionospheric maps after the maximum of solar cycle 24
IAACs | CODE | ESA/ESOC | JPL | UPC-IonSAT | CAS* | EMR/NRCan* | WHU* | DGFI-TUM** |
---|---|---|---|---|---|---|---|---|
Method | SH (15 × 15) | SH (15 × 15) | Three-shell model | Tomography + Splines/Kriging | SHPTS | SH (15 × 15) | SH (15 × 15) | B-Splines |
GNSSs | G + R | G + R | G + R | G | G + R + C | G + R | G + R | G + R |
Predicted GIMs | × (1, 2, 5 d) | × (1, 2 d) | n/a | × (2 d) | × (1, 2, 5 d) | n/a | n/a | n/a |
Rapid and final GIMs | × (1 h) | × (2 h) | × (2 h) | × (15 min, 1, 2 h) | × (30 min) | × (1 h) | × (2 h) | × (15 min, 2 h) |
RT-GIMs | n/a | n/a | n/a | × (15 min) | × (5 min) | n/a | n/a | n/a |
References | Feltens (2007) | Hernández-Pajares et al. (1999), Orús et al. (2005), García-Rigo et al. (2011) | Ghoddousi-Fard et al. (2011) | Zhang and Zhao (2018) |