receiver specific and depends significantly on its 
quality. 
4.4 Comparison with Simulations 
Comparing these observations with the theoretical 
values determined by Monte Carlo simulations (listed 
in brackets in table 2) shows that in urban areas the 
real error distribution lies somewhere between that of 
a fully random distribution (ratio 50%) and that of the 
covariance matrix (ratio 54%). 
 
Figure 7: Dependence of the predictions performances on 
the distributions deformation (Monte Carlo simulations). 
All other scenarios lie well above the theoretical 
value, proving that the covariance matrix is not only 
strongly correlated to the real error distribution in 
open sky areas, but also that higher axis ratios would 
describe it better with the same inclination angles, 
hinting systematic errors. Since this behaviour 
occurred equally for varying experimental conditions 
(e.g. speed, driving direction, satellite constellations, 
daytime, etc.) it can most probably be traced back to 
the receivers themselves. Many receivers rely on the 
weighted least squares method, which weights the 
used satellites independently. In single-frequency 
SPS receivers the pseudorange error measurements, 
dominated by ionospheric effects, can be 
approximated by the satellites’ elevations (Kaplan, 
2005, 332). This results in higher deformations of the 
error distriutions. The same conclusions apply to the 
relative resolution of the analysed error estimations.  
5 CONCLUSION 
The main purpose of this work was to compare 
different error distributions of the GNSS localization 
derived from the satellite constellation. Field tests 
were performed in characteristic scenarios, at varying 
conditions, daytimes, and test receivers. It could be 
shown that while shadowing has a positive effect on 
the distributions’ eccentricity and thus on the 3PEs 
relative accuracy, multipath propagation leads to the 
opposite result. The latter could be attributed to the 
distortion of the DOP matrix due to satellites 
erroneously taken into account. In open sky areas 
however, the 3PE estimation proved to perform 
considerably better than the simplified error 
distributions. Furthermore, the magnitude of this 
effect seemed to be correlated to the used test 
receiver. Cheaper receivers incorporate fewer 
satellites into their fixes, yielding more deformed 
error distributions. The gain of accuracy per 
transmitted parameter is thus notably higher than in 
expensive super accurate receivers. Simulations 
supported the experimental results; nevertheless, 
further research is highly encouraged. 
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