EGU26-17739, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-17739
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Monday, 04 May, 14:00–15:45 (CEST), Display time Monday, 04 May, 14:00–18:00
 
Hall X2, X2.13
Single station experiments with ASO304 data
Thibault Deleu, Yuting Cheng, Ozgur Karatekin, and Alime Ozyildirim
Thibault Deleu et al.
  • Royal Observatory of Belgium, Reference systems and planetology, Uccle, Belgium (thibault.deleu@observatory.be)

Satellite observation is becoming more and more relevant to geodetic VLBI since the Genesis is coming up. The Genesis satellite will carry a VLBI transmitter emitting broadband signals in S, C and X bands. A mode with a PRN code is proposed to enable single station measurements. We explore the potential of such measurement by analyzing real data. In the experiment ASO304, the Australian VGOS telescopes tracked five GPS satellites using their L band capability. We correlate these data with a GNSS-like approach — correlating with local replicas instead of interferometry. We perform systematic analysis on the obtained delays to characterize potential performance and error sources, in preparation for the assessment of single station operation possibility of the Genesis mission.

How to cite: Deleu, T., Cheng, Y., Karatekin, O., and Ozyildirim, A.: Single station experiments with ASO304 data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17739, https://doi.org/10.5194/egusphere-egu26-17739, 2026.