2D MHD simulations with self-consistent reconnection heating support the claim that the height of localized chromospheric heating selects between the evaporation-condensation and direct injection routes to solar prominence formation.
¨Uber den Einfluß der Eigenrotation der Zentralk¨ orper auf die Bewegung der Planeten und Monde nach der Einsteinschen Gravitationstheorie,
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A unified model of solar prominence formation with self-consistent heating
2D MHD simulations with self-consistent reconnection heating support the claim that the height of localized chromospheric heating selects between the evaporation-condensation and direct injection routes to solar prominence formation.