Solar prominences: theory and models
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 cor...
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| Format: | Article |
| Language: | English |
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Springer
2018-10-01
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| Series: | Living Reviews in Solar Physics |
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| Online Access: | http://link.springer.com/article/10.1007/s41116-018-0016-2 |