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The Rayleigh—Taylor instability as a trigger of solar flares

The review of authors’ papers is devoted to the essential role of the Rayleigh—Taylor instability (RTI) as a trigger of flare energy release. We have analyzed two cases of RTI: near coronal loop footpoints and at the loop top. RTI near loop footpoints requires pre-heating of chromospheric plasma. Th...

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Autors principals: Stepanov Aleksandr, Zaitsev Valeriy
Format: Artigo
Idioma:Inglês
Publicat: INFRA-M 2025-09-01
Col·lecció:Solar-Terrestrial Physics
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Accés en línia:http://doi.org/10.12737/stp-113202513
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