Conditions for Solar Prominence Formation Triggered by Single Localized Heating

We performed numerical simulations to study mechanisms of solar prominence formation triggered by a single heating event. In the widely accepted “chromospheric-evaporation condensation” model, localized heating at footpoints of a coronal loop drives plasma evaporation and eventually triggers condens...

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Veröffentlicht in:	The Astrophysical journal 2025-01, Vol.978 (1), p.94
Hauptverfasser:	Yoshihisa, Takero, Yokoyama, Takaaki, Kaneko, Takafumi
Format:	Artikel
Sprache:	eng
Schlagworte:	Magnetohydrodynamics Solar corona Solar prominences
Online-Zugang:	Volltext
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