Abstract
Regardless of how a prominence is formed, once it exists, we are faced with the problem of devising a model that can describe its appearance and behavior. Closely linked to this problem is the question of the stability of the prominence and of how the prominence is maintained or developed.
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© 1995 Springer Science+Business Media Dordrecht
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Tandberg-Hanssen, E. (1995). Prominence Models. In: The Nature of Solar Prominences. Astrophysics and Space Science Library, vol 199. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3396-0_5
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DOI: https://doi.org/10.1007/978-94-017-3396-0_5
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-4526-3
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