Simulation data from "Dynamic modeling of coronal abundances during flares on M-dwarf stars"
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Simulation data and code used to create the plots from the paper by Brooks et al., entitled "Dynamic modeling of coronal abundances during flares on M-dwarf stars". The code has been modified in the enhanced high-FIP case to change the abundances of elements with FIP > 10 eV.
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Zenodo创建时间:
2025-09-30



