EGU26-17126, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-17126
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, X2.11
The Vienna VLBI and Satellite Software VieVS: Status and Roadmap
Sigrid Böhm1, Johannes Böhm1, Jakob Gruber2, Frederic Jaron1, Lisa Kern1, Hana Krásná1, Matthias Schartner3, Peter Urban1, Marcus Franz Wareyka-Glaner1, and Helene Wolf1
Sigrid Böhm et al.
  • 1Department of Geodesy and Geoinformation, TU Wien, Vienna, Austria (sigrid.boehm@tuwien.ac.at)
  • 2BEV - Federal Office of Metrology and Surveying, Vienna, Austria
  • 3Department of Civil, Environmental and Geomatic Engineering, ETH Zürich, Zurich, Switzerland

Since its launch by the VLBI group at TU Wien in 2008, the Vienna VLBI and Satellite Software VieVS has grown considerably. What began as pure VLBI analysis software has evolved into a powerful conglomerate of various modules. The VLBI capabilities include a tool for simulating raw telescope data and the VLBI core module, with observation data simulation, analysis of source and satellite observations, and global solution options. The previously integrated scheduling tool was separated from VieVS-VLBI and further developed as a full-fledged standalone scheduling and simulation software, VieSched++, which is currently maintained at ETH Zurich. In addition to the VLBI-related modules, VieVS offers a tropospheric ray-tracing package called RADIATE. Another highlight is the independent open-source software package raPPPid for Precise Point Positioning, which enables the processing of low-cost or high-quality GNSS observations in highly adaptable PPP approaches. In this contribution, we provide an overview of all current open-source components of VieVS and give a preview of two new modules that will be publicly available in the future. These are VieCompy, a stand-alone combination software for estimating global parameters based on normal equations, and VieSOFT, a tool for correcting source structure at fringe-fitting level, which can also be used for correcting VLBI observations to the Genesis satellite.

How to cite: Böhm, S., Böhm, J., Gruber, J., Jaron, F., Kern, L., Krásná, H., Schartner, M., Urban, P., Wareyka-Glaner, M. F., and Wolf, H.: The Vienna VLBI and Satellite Software VieVS: Status and Roadmap, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17126, https://doi.org/10.5194/egusphere-egu26-17126, 2026.