Solar prominences: theory and models

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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Bibliographic Details
Main Author: Sarah E. Gibson
Format: Article
Language:English
Published: Springer 2018-10-01
Series:Living Reviews in Solar Physics
Subjects:
Solar prominences
Magnetohydrodynamics
Corona: structures
Prominences: Magnetic fields
Prominences: Models
Online Access:http://link.springer.com/article/10.1007/s41116-018-0016-2

Internet

http://link.springer.com/article/10.1007/s41116-018-0016-2

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