EGU2020-13256
https://doi.org/10.5194/egusphere-egu2020-13256
EGU General Assembly 2020
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Improved SLR orbit validation for Copernicus Sentinel-3 mission

Marc Fernández1, Virginia Raposo1, Jaime Fernández Sánchez1, Heike Peter2, and Pierre Féménias3
Marc Fernández et al.
  • 1GMV AD., Isaac Newton 11, 28760 Tres Cantos, Spain
  • 2PosiTim UG, In den Löser 15, 64342 Seeheim-Jugenheim, Germany
  • 3ESA/ESRIN, Largo Galileo Galilei 1, I-00044 Frascati, Italy

The European Copernicus Sentinel-3 mission, a jointly operated mission by ESA and EUMETSAT, consists of two satellites equipped with GPS and DORIS receivers, and a Laser Retro Reflector (LRR) array, which allows tracking the satellites by Satellite Laser Ranging (SLR). The SLR observations are mainly used for the validation of GPS- and/or DORIS-derived precise orbit solutions. The SLR residuals are derived from the simple difference between observed and computed range between SLR station and the satellite. Only a subset of the SLR stations tracking the satellites is normally used for this purpose. The subset consists of stations delivering good quality observations on a long-term. The station selection is regularly reviewed to guarantee a continuous quality for the orbit validation.

Instead of using only a subset of the stations it would be preferable to use as many laser tracking data as possible. Long-term and highly accurate orbit time series of low Earth orbiting satellites can be used to estimate station range biases. The SLR validation is significantly improved by adding these station range biases due to additional stations and due to the removal of SLR related systematic patterns.

In the Copernicus POD Service (CPOD), the SLR station range biases are estimated based on a combined Sentinel-3A and -3B orbits computed from different orbit providers (the CPOD Quality Working Group). Performance, quality, mission dependency and stability of these SLR station range biases are analysed based on operational CPOD orbits and orbit solutions delivered by the Copernicus POD Quality Working Group.

How to cite: Fernández, M., Raposo, V., Fernández Sánchez, J., Peter, H., and Féménias, P.: Improved SLR orbit validation for Copernicus Sentinel-3 mission, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-13256, https://doi.org/10.5194/egusphere-egu2020-13256, 2020

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