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Xia et al. Satell Navig             (2021) 2:8                                        Page 11 of 19





                                                              Static positioning analysis
                                                              Figure 14 illustrates the number of tracked satellites and
                                                              GDOP values for each constellation during the two-hour
                                                              static observation period.
                                                                At the epoch of the 4230th second in the top panel the
                                                              number  of the  tracked satellites  is zero.  Tis  indicates
                                                              that the smartphone loses lock of all satellites. From the
                                                              fgure, GPS satellites have the best visibility at the static
                                                              site with an average of about 10.0 visible satellites. BDS is
                                                              in the second with an average number of 8.2. Before the
                                                              5455th  second,  the  number  of  visible  satellites  remains
                                                              about 8–9, but declines afterwards as some satellites drop
                                                              below the elevation cutof angle. Galileo has the small-
                                                              est number of visible satellites with an average of 4.8,
                                                              although the number is relatively stable for most of the
                                                              time. Teir GDOP values give a consistent interpretation.
                                                              Te ascending order of the overall GDOP value is GPS,
                                                              GLONASS,  BDS  and  Galileo,  and  their  average  GDOP
                                                              are 1.8, 2.5, 2.7 and 9.7, respectively. Te GDOP value of
                                                              BDS increases signifcantly between the 6745th second
                                                              and the 6935th second due to a decrease in the number
                                                              of valid satellites, which raises  its overall GDOP value.
                                                              Galileo has very large GDOP values at the beginning and
              Fig. 10  Histogram and statistics of the C/N0 measurements of a
              BDS-2 and b BDS-3 satellites at elevation angles above 45°  does not return to a relatively ideal geometry state until
                                                              the 2031st second, but its GDOP is still the largest among
                                                              the four systems for the rest of the time.
                                                                Figure  15 shows the relative horizontal locations
            satellite clock bias calculated using the broadcast ephem-  obtained using the pseudorange observations of diferent
                           2
                  S
                        S
            eris;  γ = f /f  S   is the frequency-dependent scale   systems and their combination.
                  j    1  j
            factor.                                             Te average value of GLONASS positioning results is
              Te SPP solutions were obtained by adopting the   selected as the origin of the topocentric coordinate sys-
            weighted least squares (WLS) method based on satellite   tem. Although there is no ground-truth value, we can
            elevation angle, and the stochastic model is as follows   evaluate the positioning performance by analyzing the
            (Takasu and Yasuda 2009):                         dispersion of each set of positioning results. It is clearly
                                                              seen that GLONASS has the worst positioning results

                           −2  −2     −2                      due to its inconsistent ranging precision and inter-fre-
                W = diag σ   , σ  , . . . , σ            (5)
                           1   2      n
                                                              quency code bias (Reußner and Wanninger  2012). In
                                                              contrast, there are much better concentrations of BDS,

                                              2
                                  2
                  2
                                        2
                         2
                                                         2
                             2
                                                   2
                σ = F S  a + b /sin θ + σ eph  + σ ion  + σ trop  + σ bias  GPS and Galileo positioning results. Te positioning
                         σ
                             σ
                                                         (6)  precision of BDS and GPS in the east direction is better
                                                              than that in the north direction, while Galileo position
            where F  is the satellite system error factor (1: BDS, GPS   solutions are very close together in the north direction
                   S
            and Galileo, 1.5: GLONASS);  a σ and b σ are code error   but scattered in the east direction. Since the position-
            factors; θ is the satellite elevation angle; σ 2   is the vari-
                                               eph            ing results of GLONASS are not satisfactory, it is not
            ance of ephemeris and clock error; σ 2   is the variance of   included in the multi-system SPP solutions. Te fgure
                                           ion
            ionosphere correction model error; σ 2   is the variance   shows that the fusion of BDS B1, GPS L1 and Galileo
                                            trop
                                               2
            of troposphere correction model error; σ bias  is the vari-  E5a code observations signifcantly improve the posi-
            ance of code bias error. For the reliable position solutions   tioning precision, which is thanks to the increase in
            the Chi-square test was employed to verify the results.   the  number  of  valid  satellites  and  the  enhancement
            When the test fails, the position solution at that epoch is   of geometric distribution of satellites. Te concentra-
            discarded. Te elevation cutof angle of the satellite was   tion of the position solutions is high and there are no
            all set to 10°.                                   obvious outlying points. Te increased availability of
                                                              positioning results from a multi-constellation system
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