Thermodynamic and magnetic evolution of an eruptive C-class solar flare observed with SST/TRIPPEL-SP

Solar flares are complex phenomena driven by the release of magnetic energy, but a large energy reservoir is not sufficient to determine their eruptive potential; the magnetic topology and plasma dynamics play a key role. We investigated the thermodynamic and magnetic properties of the solar atmosph...

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Principais autores:	Díaz Baso C. J., de la Cruz Rodríguez J., Doerr H.-P., van Noort M., Prasad A., Feller A., Kiselman D.
Formato:	Artigo
Idioma:	Inglês
Publicado em:	EDP Sciences 2026-03-01
Colecção:	Astronomy & Astrophysics
Assuntos:	radiative transfer techniques: polarimetric sun: atmosphere sun: chromosphere sun: flares sun: magnetic fields
Acesso em linha:	https://www.aanda.org/articles/aa/full_html/2026/03/aa57756-25/aa57756-25.html
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