From: GSTAR: an innovative software platform for processing space geodetic data at the observation level
Items | Descriptions |
---|---|
Sample rate | 30Â s |
Cutoff elevation | 1° |
Observation | Undifferenced ionosphere-free linear combination of code and phase measurements on GPS L1/L2 |
Observation weighting | A priori precision of 5Â mm for SLR observations, and a priori precision of 0.3Â m and 2Â mm for GPS raw code and phase observations |
GPS orbit and clock | Products released by WHU |
Observation-specific signal bias | Products released by WHU (Geng et al., 2022) |
On-board GPS antenna phase center location vector | Values provided by Save (2019) |
On-board laser retroreflector array coordinate | Values provided by Save (2019) |
Tropospheric delay | For SLR, corrected via Mendes and Pavlis (2004) For LEO on-board GPS, not considered |
SLR range bias | Estimated as constant for each station per day (Couhert et al., 2018) |
GRACE-FO satellite attitude | Quaternion products |
Earth gravity | European Improved Gravity model of the Earth by New techniques (EIGEN6C) (120 × 120) (Shako et al., 2014) |
Solar radiation pressure | Macro-model |
Atmospheric drag | Drag Temperature Model (DTM 94) is applied (Berger et al., 1998); Piecewise constant coefficients of atmospheric drag are estimated with an interval of 90Â min |
Earth radiation pressure | Not considered |
Empirical acceleration | Piecewise periodical parameters in the along-track and cross-track directions are estimated with an interval of 90Â min |