EGU22-2383
https://doi.org/10.5194/egusphere-egu22-2383
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

Investigation of the flicker nature of the day-boundary differences of GNSS orbits

Hanane Ait-Lakbir1, Alvaro Santamaria1, Félix Perosanz1, and Jim Ray2
Hanane Ait-Lakbir et al.
  • 1GET, Université Paul Sabatier, CNES, CNRS, IRD, UPS, Toulouse, France
  • 2National Geodetic Survey (retired), Silver Spring, MD, USA

Day-boundary orbit comparison is one of the criteria used to assess the performance of GNSS orbits. The overall statistics of orbit discontinuities such as RMS are usually computed to assess dynamical modeling and the processing configurations. Additional information about the systematic orbit errors is also accessible through their spectral content.

A particular feature is the flicker or 1/f noise describing the low-frequency band, indicating time-correlated orbital errors. This type of noise is observed not only in the orbits but also in other GNSS-derived geodetic time series such as in station positions, Earth rotation parameters,... The sources explaining this feature, either from the GNSS orbit modeling or from unaccounted orbital perturbations, are not well understood. By computing simulated orbits, we look at possible causes in the orbit determination processing.

How to cite: Ait-Lakbir, H., Santamaria, A., Perosanz, F., and Ray, J.: Investigation of the flicker nature of the day-boundary differences of GNSS orbits, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-2383, https://doi.org/10.5194/egusphere-egu22-2383, 2022.