The new-generation geodetic radio telescopes observe two orthogonal linear polarization directions. Calibration of the gain differences between the two polarizers is necessary to maximize the signal-to-noise ratio of observations. This study investigates these cross-polarization gain differences and their temporal evolution for selected antennas. Check it out!
Recent Posts
- Vienna VLBI Group at IAG Scientific Assembly 2025
- Paper on Atmospheric Excitation of Length of Day Inferred From 21st Century Climate Projections published
- Vienna VLBI Group at EVGA 2025
- Department Seminar at Masaryk University in Brno
- Paper on Terrestrial Reference Frame Scale Drift Anomalies in VLBI published
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TU Wien
Department of Geodesy and Geoinformation
Research Division Higher Geodesy
Wiedner Hauptstraße 8-10, 1040, Vienna
Austria
Contact Information
Email: vlbi_contact@tuwien.ac.at



