Thermal instability in coronal loops: Linking eigenvalue spectra to time-dependent evolution

Context. Cool, dense condensations such as coronal rain and prominences suggest that coronal plasma can undergo runaway radiative cooling. Connecting this behaviour to linear thermal modes requires a fuller understanding of the deeper connection between eigenvalue spectra and actual time-dependent e...

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Hlavní autoři:	Kelly Adrian, Keppens Rony, De Jonghe Jordi
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	EDP Sciences 2026-06-01
Edice:	Astronomy & Astrophysics
Témata:	hydrodynamics instabilities magnetohydrodynamics (mhd) methods: numerical sun: corona sun: filaments prominences
On-line přístup:	https://www.aanda.org/articles/aa/full_html/2026/06/aa59934-26/aa59934-26.html
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