Modeling atmospheric transport of cosmogenic radionuclide ¹⁰Be using GEOS-Chem 14.1.1 and ECHAM6.3-HAM2.3: implications for solar and geomagnetic reconstructions<b> </b>

Model outputs for the paper "Modeling atmospheric transport of cosmogenic radionuclide ¹⁰Be using GEOS-Chem 14.1.1 and ECHAM6.3-HAM2.3: implications for solar and geomagnetic reconstructions"<br>It includes the model outputs from the ECHAM6.3-HAM2.3 ("E63H23" folder) and GEOS-Chem 14.1.1 ("GEOS-Chem" folder) using the Beryllium production model by Poluianov et al., (2016).The model outputs are averaged over the period 2005-2013. Both "E63H23" and "GEOS-Chem" folders have the following subfolders- "CONTROL" folder: simulations with production rates using Phi from the Herbst et al., (2017) and spatial geomagnetic cut-off rigidity from Copeland (2018).- "Solar_minimum_200MeV" folder: simulations with production rates using constant Phi=200 MeV and spatial geomagnetic cut-off rigidity from Copeland (2018).- "Geomagnetic_minium_Laschamps" folder: simulations with production rates using constant Phi=500 MeV and spatial geomagnetic cut-off rigidity from generated by the geomagnetic field model LSMOD.2 at the period 40.95 ka (Gao et al., 2022).