Exploring reasons for the ITRF2020 VLBI scale drift
Paper in proceeding, 2023

Since the release of the new realisation of the International Terrestrial Reference System, ITRF2020, one of the focuses of the IVS community is to understand the cause of the drift in the VLBI scale factor time series after 2013.75 that is detected by the ITRF team.
In this work, we consider the official IVS combined solution, i.e. the IVS contribution to the ITRF2020 realisation, and calculate scale factors using the CATREF software with the single-technique combination strategy that was used to process the ITRF2020.
The investigation of time series of Up components of specific IVS stations with the statistical tool BEAST reveals offsets and trends changes that are not taken into account in the ITRF2020.
These changes are significant for five IVS stations: NYALES20, WETTZELL, ONSALA60, TSUKUB32, and MATERA.
Adding discontinuities for these five IVS stations significantly decreases the VLBI scale drift.

ITRF

VLBI scale drift

BEAST

CATREF

Author

Karine le Bail

Chalmers, Space, Earth and Environment, Onsala Space Observatory

Masafumi Ishigaki

Geospatial Information Authority of Japan

Rüdiger Haas

Chalmers, Space, Earth and Environment, Onsala Space Observatory

Tobias Nilsson

The Swedish Mapping, Cadastral and Land Registration Authority

Maxime Mouyen

Chalmers, Space, Earth and Environment, Onsala Space Observatory

Proceedings of the 26th Meeting of the European VLBI Group for Geodesy and Astrometry (EVGA)

26th Meeting of the European VLBI Group for Geodesy and Astrometry
Bad Kötzting, Germany,

Subject Categories (SSIF 2025)

Earth and Related Environmental Sciences

DOI

10.14459/2023md1730292

More information

Latest update

1/16/2026