“…6 mm (given with typical level) [35] After the distance-dependent errors, namely the DD atmospheric delays and orbital errors, are reduced by the processing strategy in Table 4, the number and distribution of visible satellites, i.e., Inter-satellite-type bias Homogenous receivers (Trimble R9) [34] Observation weighting σ ∆∇P = 60 cm, σ ∆∇Φ = 6 mm (given with typical level) [35] After the distance-dependent errors, namely the DD atmospheric delays and orbital errors, are reduced by the processing strategy in Table 4, the number and distribution of visible satellites, i.e., satellite geometry, and measurement noises including multipath are the major factors affecting ambiguity resolution [36][37][38]. To reflect the influence of code noise on ambiguity resolution, we need to select some test sessions whose code noises are visibly different.…”