Exploring reasons for the ITRF2020 VLBI scale drift
Paper in proceeding, 2023
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)
Bad Kötzting, Germany,
Subject Categories (SSIF 2025)
Earth and Related Environmental Sciences
DOI
10.14459/2023md1730292