Identification of system-specific observation errors for SLR and VLBI telescopes at GOW
- 1Deutsches Geodätisches Forschungsinstitut (DGFI-TUM), Technical University of Munich, Munich, Germany
- 2Geodätisches Observatorium Wettzell, Forschungseinrichtung Satellitengeodäsie, Technical University of Munich, Munich, Germany
- 3Geodätisches Observatorium Wettzell, Bundesamt für Kartographie und Geodäsie, Frankfurt, Germany
The observations of the four space-geodetic techniques (GNSS, SLR, VLBI, DORIS) are used for the computation of the International Terrestrial Reference Frame (ITRF) and for the realisation of its geodetic datum as well as (except VLBI) for the precise orbit determination of Earth-observing satellites. The ITRF itself is fundamental for a broad variety of scientific and societal applications such as Earth monitoring and positioning, relevant for satellite companies, logistics, and finally new techniques like autonomous driving. However, all four techniques still suffer from unknown systematic measurement or modelling errors which makes the estimation of bias parameters inevitable.
The Geodetic Observatory Wettzell (GOW), Germany, with its unique and ideal test environment comprising multiple GNSS antennas, three VLBI antennas, two SLR telescopes, a DORIS beacon, and numerous other sensor systems provides the opportunity to systematically identify, quantify, understand, and compensate system-specific measurement errors. The installation of a so-called common target (CT) in 2017 and the realisation of a common clock (CC) enables a profound analysis of space-geodetic measurements. The CT is connected to the clocks of the space-geodetic techniques via delay-compensated fibre links which allows so-called ‘closure in time’ experiments.
Within the recently established DFG research unit ‘Clock Metrology: Time as a New Variable in Geodesy’, one project at DGFI-TUM focuses on the investigation of time-related and technique-specific errors using ‘closure in time’ experiments at the GOW. Therefore, completed experiments involving the CT are analysed and enhanced experiments will be planned and conducted. With the aid of the CC, the source of present measurement discrepancies will be investigated and resolved. We present the current state of our work with the main focus on the analysis of VLBI and SLR observations of the two SLR and three VLBI systems at GOW.
How to cite: Zeitlhöfler, J., Bloßfeld, M., Neidhardt, A., and Eckl, J.: Identification of system-specific observation errors for SLR and VLBI telescopes at GOW, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-10691, https://doi.org/10.5194/egusphere-egu24-10691, 2024.
