Dataset for "Necessary core-mantle boundary heat flux patterns for large latitude of geomagnetic surface intensity minima" by "Terra-Nova, F. and Amit, H."

CMB spherical harmonics of the magnetic field of our numerical dynamo simulation using Gastine, T., Barik, A., Rraynaud, Schwaiger, T., Putigny, B., T., Wicht, J., LDVDuarte, Dintrans, B., 2022. magic-sph/magic: release magic 6.2 (v6.2). Zenodo 211 (1),821 https://doi.org/10.5281/zenodo.7419346.

Those are B_coeffs files (for details please consult https://magic-sph.github.io/outputFiles/outCoeffFiles.html) that can be used to reproduce our results in Terra-Nova and Amit (Submitted, JGR). Consult there Table 1 for the control parameters of the simulations. 

We also publish here input files of the MagIC code for each heat flux pattern imposed on the outer boundary. Those allow the complete reproduction of our results using MagIC code (Gastine et al., 2022).

For futher data set sharing please communicate via filipe.terranova@univ-nantes.fr.