Published July 16, 2026 | Version v6
Dataset Open

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)

Name Size
md5:39212371fbb133313fa6d53836671ea8
24.9 GB Preview Download

Additional details

Funding

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