Diagnostics of the solar atmosphere and its stellar context
This project aims to push forward our present understanding on the magnetism and dynamics of the solar atmosphere through the interpretation of observational data with inference methods. We approach the study of the solar atmosphere stressing its connectivity by magnetic fields and dynamical processes. We also emphasise the solar-stellar connection
María Jesús
Martínez González
Íñigo
Arregui Uribe-Echevarría
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