Abstract
Tracking L-band signals of GNSS satellites by radio telescopes became a new observation type in recent years and will be used to improve reference system realizations and links between Earth- and space-fixed frames. First successful test observations were done, with the drawback of being single-frequency only. In order to correct the ionospheric delay by using GNSS phase observations from co-located receivers, the L4R approach was developed. Based on residuals derived by a least-squares processing of the GNSS geometry-free linear combination corresponding corrections could be derived. As a first validation step L4R corrections were applied to GNSS \(L_1\) data analysis. Station coordinate repeatibilities at the 1-cm level were obtained for baselines of a few thousand kilometers. Comparing the derived delay corrections to VLBI ionospheric delays for quasars located in same directions, differences with a standard deviation of 2.2 TECU could be achieved.
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Notes
With respect to a magnetic reference frame (latitude of the geomagnetic north pole is 87.2\(^\circ \) N).
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Acknowledgments
The authors want to thank IVS and IGS for providing the necessary observations and CODE and TU Vienna for providing GNSS and atmospheric products allowing a suitable processing. They would also like to thank three anonymous reviewers for their assistance in evaluating this paper and their helpful recommendations. This work was done within the project “Co-location of Space Geodetic Techniques on Ground and in Space” which is part of the DFG funded Research Unit “Space-Time Reference Systems for Monitoring Global Change and for Precise Navigation in Space” (FOR 1503).
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Männel, B., Rothacher, M. Ionospheric corrections for single-frequency tracking of GNSS satellites by VLBI based on co-located GNSS. J Geod 90, 189–203 (2016). https://doi.org/10.1007/s00190-015-0865-6
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DOI: https://doi.org/10.1007/s00190-015-0865-6