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Data-driven modeling of solar coronal magnetic field evolution and eruptions
Magnetic fields play a fundamental role in the structure and dynamics of the solar corona. As they are driven by their footpoint motions on the solar surface, which transport energy from the interior of the Sun into its atmosphere, the coronal magnetic fields are stressed continuously with buildup o...
| Autores principales: | , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Elsevier
2022
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9035809/ https://www.ncbi.nlm.nih.gov/pubmed/35479733 http://dx.doi.org/10.1016/j.xinn.2022.100236 |