Solar prominences: theory and models
| Autor: | Sarah E. Gibson |
|---|---|
| Jazyk: | angličtina |
| Rok vydání: | 2018 |
| Předmět: | |
| Zdroj: | Living Reviews in Solar Physics, Vol 15, Iss 1, Pp 1-39 (2018) |
| Druh dokumentu: | article |
| ISSN: | 2367-3648 1614-4961 |
| DOI: | 10.1007/s41116-018-0016-2 |
| Popis: | Abstract 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 understanding from observations that give us information about the structure of the “magnetic skeleton” that supports and surrounds the prominence. Energetically-sophisticated magnetohydrodynamic simulations then add flesh and blood to the skeleton, demonstrating how a thermally varying plasma may pulse through to form the prominence, and how the plasma and magnetic fields dynamically interact. |
| Databáze: | Directory of Open Access Journals |
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