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Carrier phase ambiguity fixing with two frequencies

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FundamentalsFundamentals
Title Carrier phase ambiguity fixing with two frequencies
Author(s) J. Sanz Subirana, J.M. Juan Zornoza and M. Hernández-Pajares, Technical University of Catalonia, Spain.
Level Advanced
Year of Publication 2011
  • A simple approach for ambiguity fixing is presented briefly as follows [footnotes 1]:


Wide-lane ambiguity fixing: The double-differenced wide-lane ambiguity can be computed from the Melbourne Wübbena Combination, by rounding the average in time [footnotes 2] (see equations in the article Combining pairs of signals and clock definition).
This ambiguity estimate has the advantage that it can be obtained separately for each measurement, easily, thanks to the enlargement of the ambiguity spacing. Under moderate receiver noise and multipath conditions, a few minutes should be enough to fix the wide-lane ambiguity.


L1 ambiguity fixing: After fixing the double differenced L1 ambiguity () can be fixed from the expression


when an estimate of the ambiguity accurate enough is available. This estimate can be computed as in the previous section (PPP), floating the ambiguities in the Kalman filter.


As the ambiguities are determined "by floating" them in the navigation filter, some time span is needed (most part of one hour) for the filter to be converged. Indeed, roughly speaking, this ambiguity is mostly estimated from , where the code noise is about three times noisier than the code measurement in the frequency (see Figure 1 corresponding to GNSS Measurement features and noise).


Figure 1:GPS code and carrier phase measurement features. The geometry-free combinations of code (), in green, and carrier (), in blue, are plotted as function of time for a given satellite.


There are more sophisticated methods as the Lambda Method (see [Teunissen, 1996] [1], [Teunissen et al., 1997][2]) or the Null Space (see [Martin-Neira et al., 1995] [3]), among others [Kim and Langley, 2000] [4], where the ambiguities are fixed "as a set", and decorrelation and search (on integers) techniques are applied to enhance the ambiguity resolution.


Ionosphere-free bias fixed: After fixing the and ambiguities, the double differenced ionosphere-free bias is fixed by:


Notice that, once the ambiguity is fixed, thence a double-differenced measurement two orders of magnitude more accurate than the code (typically) is available to navigate. This allows to achieve centimetre level of positioning accuracy.


  • An alternative way to avoid the time span needed for the floated to converge is to use the following equation, for the ambiguity fixing:


The main problem here is the ionospheric refraction term .


For short baselines (up to kilometres, depending on the ionospheric conditions) it can be assumed that the double-differenced ionospheric refraction cancels, i.e., , and thence, the ambiguity can be fixed by rounding from the expression:


This is the approach applied in the RTK ambiguity fixing technique.


For long baselines, an accurate ionospheric correction estimate is needed to allow the user to fix the ambiguity by rounding from (4). Notice that, once the ambiguity is fixed, being the carrier measurement noise of few millimetres, the main contribution to the rounding error is from the term. Notice also that its accuracy must be better than to allow the integer rounding. In the case of the Galileo E1 and E5b signals, this accuracy threshold is , (see Table 1 in the article Carrier phase ambiguity fixing with three frequencies). For the of L1 and L2 GPS signals, it is , see table in the article Combination of GNSS Measurements).


The WARTK technique has proved that accurate ionospheric corrections can be computed from the measurements gathered from permanent reference stations networks with similar baselines as SBAS (WAAS, EGNOS, …) networks. Such highly accurate ionosphere allows the carrier phase ambiguity fixing over a wide area. In this way, the WARTK technique can allow to extend the RTK ambiguity fixing from local area to wide-area, i.e., at continental scale. See more details in the following references [Hernandez-Pajares et al., 2010][5], [Hernandez-Pajares et al., 2003a] [6] and [Hernandez-Pajares et al., 2003b][7].


Notes

  1. ^ The next expressions can be easily derived from the equations presented in the article Combining pairs of signals and clock definition
  2. ^ Notice that the code noise is reduced in the narrow-lane combination by a factor , (see GNSS Measurement features and noise), and on the other hand the ambiguity spacing is wider in the wide-lane combination (see Combination of GNSS Measurements) and figures in the articles GNSS Measurement features and noise Detector based in code and carrier phase data: The Melbourne-Wübbena combination respectively). For instance, for Galileo E1, E5b signal, the (see Table 1 in Carrier phase ambiguity fixing with three frequencies), or for the L1, L2 GPS signals the (see table in Combination of GNSS Measurements).

References

  1. ^ [Teunissen, 1996] Teunissen, P., 1996. GPS Carrier phase ambiguity Fixing concepts, in GPS for Geodesy. Lecture Notes in Earth Sciences, Springer. pp. 263-335.
  2. ^ [Teunissen et al., 1997] Teunissen, P., De Jonge, P. and Tiberius, J., 1997. Performance of LAMBDA Method for Fast GPS Ambiguity Resolution. Navigation. 44(3), pp. 373-383.
  3. ^ [Martin-Neira et al., 1995] Martin-Neira, M., Toledo, M. and Pelaez, A., 1995. The null space method for GPS integer ambiguity resolution. Proceedings of DSNS'95, Bergen, Norway, April 24-28, Paper No. 31, 8 pp.
  4. ^ [Kim and Langley, 2000] Kim, D. and Langley, R. B., 2000. GPS Ambiguity Resolution and Validation: Methodologies, Trends and Issues. Proceedings of 7th GNSS Workshop - International Symposium on GPS/GNSS, Seoul, Korea, Nov. 30-Dec. 2, 2000.
  5. ^ [Hernandez-Pajares et al., 2010] Hernandez-Pajares, M., Juan, M., Sanz, J.,Aragon-Angel, A., Samson, J., Tossaint, M., Odijk, D., Teunissen, P.,De Bakker, P., Verhagen, S. and Van der Marel, H., 2010. Wide-Area RTK. InsideGNSS (March/April 2010). 5(2), pp. 36-46.
  6. ^ [Hernandez-Pajares et al., 2003a] Hernandez-Pajares, M., Juan, J., Sanz, J. and Colombo, O., 2003a. Impact of real-time ionospheric determination on improving precise navigation with Galileo and next-generation GPS. Journal of the Institute of Navigation.
  7. ^ [Hernandez-Pajares et al., 2003b] Hernandez-Pajares, M., Juan-Zornoza, J., Sanz-Subirana, J. and Colombo, O., 2003b. Feasibility of Wide-Area Subdecimeter Navigation With GALILEO and Modernized GPS. IEEE Transactions on Geoscience and Remote Sensing. 41(9), pp. 2128-2131.