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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| Hoofdauteur: | |
|---|---|
| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
Frontiers Media S.A.
2022-12-01
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| 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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