Validation of GPS III transmit antenna calibrations

Steigenberger, Peter; Thoelert, Steffen; Dach, Rolf; Montenbruck, Oliver (2023). Validation of GPS III transmit antenna calibrations. Advances in space research, 73(5), pp. 2488-2498. Elsevier 10.1016/j.asr.2023.11.048

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Accurate information about the satellite transmit antennas is essential for high-precision GNSS applications. Such metadata of the GPS III satellites were publicly made available by the manufacturer Lockheed Martin. They comprise phase center offsets (PCOs), phase patterns, and directivity patterns. These calibrations are validated with ground-based measurements of a global GPS tracking network and observations of a high-gain antenna. Phase center offsets and patterns are estimated from dual-frequency observations of a ground tracking network. The ionosphere-free L1/L2 z-PCOs show a 10 cm offset w.r.t. the manufacturer calibrations due to already known inconsistencies with the ITRF2020 scale fixed in the estimation. The standard deviation of the differences between estimated and calibrated z-PCOs is 2.7 cm. The estimated phase patterns have a 0.7 mm RMS consistency with the manufacturer calibrations after minimizing the raw patterns for nadir angles between 0° and 14°. The directivity patterns are validated with the effective isotropic radiated power (EIRP) measured with a 30 m high-gain antenna. The measured EIRP for the L1 and L2 band is affected by M-code transmission from a distinct antenna. When modeling the additional contribution of this antenna, the nadir-angle variation of the EIRP matches the calibrated directivity patterns with a precision of 0.1 dBW. Representative transmit power values of the main navigation antenna amount to 125 W, 30 W, and 85 W in the L1, L2, and L5 bands, while the L1 and L2 M-code signals are transmitted with about 30 W and 25 W, respectively.

Item Type:

Journal Article (Original Article)

Division/Institute:

08 Faculty of Science > Institute of Astronomy

UniBE Contributor:

Dach, Rolf

Subjects:

500 Science > 520 Astronomy

ISSN:

0273-1177

Publisher:

Elsevier

Language:

English

Submitter:

Daniel Arnold

Date Deposited:

03 Apr 2024 11:45

Last Modified:

05 Apr 2024 06:58

Publisher DOI:

10.1016/j.asr.2023.11.048

BORIS DOI:

10.48350/195411

URI:

https://boris.unibe.ch/id/eprint/195411

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