Option | Setting |
---|---|
Observables | DD phase and code GPS L1 and L2, Galileo E1 and E5a, BDS B1 and B2 |
Weighting scheme | Elevation-dependent weighting |
Elevation cutoff angle | 10° |
Sampling interval | 30Â s |
Sessions’ length | 15 min |
Geometry of the network, baseline selection strategy | STAR strategy with HETT as a hub station and four neighboring reference stations (KILP, KEV2, SOD3, KIR8) which constituted the reference network (Fig. 5) |
Length of the baselines in rover solution | 123–201 km |
Troposphere delay modeling | A priori delays obtained from Saastamoinen model with Global Mapping Function supported with constrained estimation of residual ZTD |
Ionosphere delay handling | Depending on the model: ionosphere-float, ionosphere-weighted, enhanced ionosphere-weighted model with RTC |
A priori variance of ionospheric parameters | Corresponding to the level of the expected residual ionospheric delays |
Solution type | Kinematic/static with ambiguity resolution |
Ambiguities handling | Fixed to integers with M-Lambda (Chang et al. 2005) |
A priori STD of observations | 0.3Â m and 0.002Â m undifferenced code and phase signals, respectively |
Satellite orbits and clocks | Broadcast |
Estimation method | Recursive least squares adjustment, forward estimation |