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Interrogating solar flare loop models with IRIS observations 1: Overview of the models, and mass flows

Solar flares are transient yet dramatic events in the atmosphere of the Sun, during which a vast amount of magnetic energy is liberated. This energy is subsequently transported through the solar atmosphere or into the heliosphere, and together with coronal mass ejections flares comprise a fundamenta...

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Bibliografische gegevens
Hoofdauteur: Graham S. Kerr
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: Frontiers Media S.A. 2022-12-01
Reeks:Frontiers in Astronomy and Space Sciences
Onderwerpen:
Online toegang:https://www.frontiersin.org/articles/10.3389/fspas.2022.1060856/full
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