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Solar prominences: theory and models: Fleshing out the magnetic skeleton
Magnetic fields suspend the relatively cool material of solar prominences in an otherwise hot corona. A comprehensive understanding of solar prominences ultimately requires complex and dynamic models, constrained and validated by observations spanning the solar atmosphere. We obtain the core of this...
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Springer International Publishing
2018
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6390890/ https://www.ncbi.nlm.nih.gov/pubmed/30872983 http://dx.doi.org/10.1007/s41116-018-0016-2 |