EGU26-9665, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-9665
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 07 May, 10:45–12:30 (CEST), Display time Thursday, 07 May, 08:30–12:30
 
Hall X2, X2.34
The updated ESA Earth System Model for Future Gravity Mission Simulation Studies: ESA ESM 3.0
Linus Shihora1, Marius Schlaak2, Volker Klemann1, Laura Jensen1, Robert Dill1, Yoshiyuki Tanaka3, Ingo Sasgen4, Bert Wouters5, Shin-Chan Han6, Jeanne Sauber-Rosenberg7, Carla Braitenberg8, Muhammad Tahir Javed8, Gerardo Maurizio8, Hugo Lecomte9, and Henryk Dobslaw1
Linus Shihora et al.
  • 1GFZ Helmholtz Centre for Geosciences, 1.3 Earth System Modelling, Potsdam, Germany (linus.shihora@gfz.de)
  • 2Technical University of Munich, School of Engineering and Design, Astronomical and Physical Geodesy , Germany
  • 3The University of Tokyo, Department of Earth and Planetary Science, Tokyo, Japan
  • 4Alfred-Wegener-Institut, Helmholtz-Zentrum für Polar- und Meeresforschung, Bremerhaven, Germany
  • 5TU Delft, Civil Engineering, Geoscience and Remote Sensing, Netherlands
  • 6Ohio State University, School of Earth Sciences, Columbus, OH, United States
  • 7NASA Goddard Space Flight Center, Geodesy and Geophysics Laboratory, Greenbelt, MD, United States
  • 8Universita' degli Studi di Trieste, Dipartimento di Matematica e Geoscienze, Trieste, Italia
  • 9Finnish Geospatial Research Institute, National Land Survey of Finland

The ESA Earth System Model (ESA ESM) provides a synthetic data set of the time-variable global gravity field that includes realistic mass variations in atmosphere, oceans, terrestrial water storage, continental ice sheets, and the solid Earth on a wide set of spatial and temporal frequencies. For more than 10 years already, it is widely applied as a source model in end-to-end simulation studies for future gravity missions, but has been also utilized to study novel gravity observing concepts on the ground. For those purposes, the ESM needs to include a wide range of signals even at very small spatial scales which might not yet have been reliably observed by any active satellite mission.

In this contribution, we present the details of the newly released version 3.0 of the ESA ESM as well as the first simulation studies based on the new model. The changes to the pervious ESA ESM version 2 include the utilization of a small ensemble of co- and post-seismic earthquake signals, an updated GIA model, additional mass balance signals from previously not considered Arctic glaciers, sub-monthly surface-mass balance changes and a more realistic representation of ice sheet dynamics. Extreme hydrometeorological events as well as climate-driven and anthropogenic impacts on continental water storage are represented through an update of the hydrological component. Additionally, the ESM separately includes ocean bottom pressure variations along the western slope of the Atlantic, representing variations in the meridional overturning circulation as a critically important component of the interactively coupled global climate system. ESA ESM 3.0 is available with 6-hour resolution from January 2007 until December 2020. It is augmented with synthetic error time series for atmosphere and ocean as well as hydrology to facilitate stochastical modelling of residual background model errors.

How to cite: Shihora, L., Schlaak, M., Klemann, V., Jensen, L., Dill, R., Tanaka, Y., Sasgen, I., Wouters, B., Han, S.-C., Sauber-Rosenberg, J., Braitenberg, C., Javed, M. T., Maurizio, G., Lecomte, H., and Dobslaw, H.: The updated ESA Earth System Model for Future Gravity Mission Simulation Studies: ESA ESM 3.0, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9665, https://doi.org/10.5194/egusphere-egu26-9665, 2026.