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Published January 3, 2026 | Version v4
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Data for 'Strengthening of the f mode due to subsurface magnetic fields in simulations of convection'

Authors/Creators

  • 1. ROR icon Inter-University Centre for Astronomy and Astrophysics
  • 2. ROR icon Institut für Sonnenphysik
  • 3. ROR icon Thüringer Landessternwarte Tautenburg
  • 4. ROR icon Friedrich Schiller University Jena

Description

Simulation output and postprocessing scripts for 'Strengthening of the f mode due to subsurface magnetic fields in simulations of convection' (https://arxiv.org/abs/2409.14840). 

Files

f_mag_str_2023.zip

Files (24.9 GB)

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md5:c307c940e811dce5f0b3e3de4b534722
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Additional details

Funding

Gauss Centre for Supercomputing
Detection of magnetic signatures with helioseismic techniques from ab initio simulations of turbulent convection 29746