Abstract
In his comprehensive book on solar prominences Tandberg-Hanssen (1974) wrote: “The single, physically most important parameter to study in prominences may be the magnetic field. Shapes, motions, and in fact the very existence of prominences depend on the nature of the magnetic field threading the prominence plasma...”
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© 1988 Kluwer Academic Publishers
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Leroy, J.L. (1988). Observation of Prominence Magnetic Fields. In: Priest, E.R. (eds) Dynamics and Structure of Quiescent Solar Prominences. Astrophysics and Space Science Library, vol 150. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3077-3_4
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DOI: https://doi.org/10.1007/978-94-009-3077-3_4
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-2834-0
Online ISBN: 978-94-009-3077-3
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