Understanding the thermal and magnetic properties of an X-class flare in the low solar atmosphere
Recently, the exploitation of spectropolarimetric data has allowed to improve our knowledge of the dynamical and magnetic response of the photospheric and chromospheric layers to the rapid release of energy occurring during solar flares. In this framework, we have used high-resolution observations acquired on 22nd October 2014 during an X1.6
Ferrente, Fabiana et al.
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2024