EGU23-5798
https://doi.org/10.5194/egusphere-egu23-5798
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Nine years of temporal gravity changes observed by the Swarm satellites

Joao de Teixeira da Encarnacao1, Arnold Daniel2, Ales Bezdek3, Christoph Dahle2,4, Junyi Guo5, Jose van den IJssel1, Adrian Jaeggi2, Jaroslav Klokocnik3, Sandro Krauss6, Torsten Mayer-Guerr6, Ulrich Meyer2, Josef Sebera3, Ck Shum5, Pieter Visser1, and Yu Zhang5
Joao de Teixeira da Encarnacao et al.
  • 1Delft University of Technology, Space Engineering, Delft, Netherlands (j.g.deteixeiradaencarnacao@tudelft.nl)
  • 2Astronomical Institute of the University of Bern, Bern, Switzerland
  • 3Astronomical Institute of the Czech Academy of Sciences, Prague, Czech Republic
  • 4GFZ German Research Centre for Geosciences, Potsdam, Germany
  • 5School of Earth Science of the Ohio State University, Columbus, Ohio, USA
  • 6Institute of Geodesy of the Graz University of Technology, Graz, Austria

Although a satellite mission to observe Earth’s magnetic field, the Swarm satellites also collect GPS data with sufficient accuracy to observe Earth’s gravity field with a spatial resolution of roughly 1500 km. These monthly models are available from 2014 to the present and do not rely on any other source of gravimetric data nor any a priori information in, for example, the form of temporal and spatial correlations. This time series covers the gap between the GRACE and GRACE-FO missions, as well as any other short gaps in their time series. Given the healthy state of the Swarm satellites, it is also likely that it will provide gravimetric information during possible gaps in the GRACE-FO data, and future dedicated gravimetric satellite missions.

We are a consortium of international research institutes, composed of the Astronomical Institute of the University of Bern, the Astronomical Institute of the Czech Academy of Sciences, the Delft University of Technology, the Institute of Geodesy of the Graz University of Technology, and the School of Earth Sciences of the Ohio State University. These activities are supported by the European Space Agency and the International Combination Service for Time-variable Gravity Fields (COST-G). We publish the models every 3 months at ESA’s Swarm Data Accessserver (https://swarm-diss.eo.esa.int) as well at the International Centre for Global Earth Models (http://icgem.gfz-potsdam.de/series/02_COST-G/Swarm). Each institute exploits different gravity inversion strategies, thus producing independent solutions, which are combined at the solution level using weights derived with Variance Component Estimation. In this way, we ensure the published models are not biased towards particular strategies or assumptions.

We illustrate the geophysical signal captured by Swarm’s GPS receivers over large hydrological basins, the errors represented by the variability of the models over the oceans and the agreement with GRACE and GRACE-FO. All analyses span the GRACE/GRACE-FO gap, to illustrate the importance of the Swarm satellites to bridge the absence of low-low satellite-to-satellite tracking data.

How to cite: de Teixeira da Encarnacao, J., Daniel, A., Bezdek, A., Dahle, C., Guo, J., van den IJssel, J., Jaeggi, A., Klokocnik, J., Krauss, S., Mayer-Guerr, T., Meyer, U., Sebera, J., Shum, C., Visser, P., and Zhang, Y.: Nine years of temporal gravity changes observed by the Swarm satellites, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-5798, https://doi.org/10.5194/egusphere-egu23-5798, 2023.