Models and Plotting Files from "Effects of geodynamo priors and geomagnetic data on inverted core surface flows"

Repository for models in "Effects of geodynamo priors and geomagnetic data on inverted core surface flows". The paper and further details about the methodology used to produce these models is available at: https://doi.org/10.1016/j.pepi.2025.107323

Authors

Hannah Rogers, Nicolas Gillet, Julien Aubert, Paolo Personnettaz, Mioara Mandea

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Acknowledgment

We thank Nathana"el Schaeffer for the access to the XSHELLS GPU code (Schaeffer, 2017; Schaeffer, 2013), to run the S1γ dynamo, and for the fruitful discussions. The S1γ dynamo computations were performed using HPC resources of IDRIS under allocation A0140407382 attributed by GENCI (Grand Equipement National de Calcul Intensif). All other dynamo performed at S-CAPAD, IPGP and using HPC resources from GENCI-TGCC and, GENCI-IDRIS and GENCI-CINES (grant number A0140402122). This work has been funded by the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (GRACEFUL Synergy Grant agreement No 855677) and by ESA in the framework of EO Science for Society, through contract 4000127193/19/NL/IA (Swarm + 4D Deep Earth: Core). It has also been partially supported by the French Space Agency (CNES) in the context of the Swarm mission of ESA. HR, NG and PP are part of Labex OSUG@2020 (ANR10 LABX56).

License

This is an open access article distributed under the terms of the Creative Commons CC-BY license, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.