EGU21-12361
https://doi.org/10.5194/egusphere-egu21-12361
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Estimation of station-dependent LRA correction parameters for the TOPEX/Poseidon mission

Julian Zeitlhöfler, Mathis Bloßfeld, Sergei Rudenko, and Florian Seitz
Julian Zeitlhöfler et al.
  • Deutsches Geodätisches Forschungsinstitut der Technischen Universität München (DGFI-TUM), Arcisstrasse 21, 80333 Munich, Germany (julian.zeitlhoefler@tum.de)

Launched in 1992, the TOPEX/Poseidon (T/P) mission is one of the first major altimetry missions. It is the predecessor of the Jason satellites which orbit the Earth on a very similar orbit. The geodetic space technique SLR (Satellite Laser Ranging) provides observations of this mission by targeting the Laser Retroreflector Array (LRA) mounted on the spacecraft. The T/P LRA is extremely large and not optimally designed. It thus causes big variations in the LRA phase center. These variations are a significant limiting factor of the orbit accuracy which makes it essential to apply a measurement correction for precise orbit determination. Up to now, only tabulated LRA corrections are available which require an interpolation.

In this contribution, we present a new approach to determine station-dependent LRA corrections to improve the phase center variations. The approach is based on a continuous analytical correction function which only uses the observation azimuth and zenith angle in combination with four parameters. These parameters are computed within an estimation process for each observing SLR station. Therefore, uncorrected SLR residuals based on raw SLR normal point observations are used. The correction value is added to the SLR measurement and counteracts the LRA phase center variations.

The advantages of this method are the continuous functional, which is easy to implement in existing software packages, as well as the avoidance of an interpolation between tabulated values. Furthermore, the differences between orbits determined with and without the LRA correction will be presented. Station coordinate time series and orbit comparisons with external T/P orbits are investigated in order to prove the high quality of the obtained LRA corrections.

How to cite: Zeitlhöfler, J., Bloßfeld, M., Rudenko, S., and Seitz, F.: Estimation of station-dependent LRA correction parameters for the TOPEX/Poseidon mission, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-12361, https://doi.org/10.5194/egusphere-egu21-12361, 2021.

Displays

Display file