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Magnetism and Dynamics of Prominences: MHD Waves

  • José Luis BallesterEmail author
Chapter
Part of the Astrophysics and Space Science Library book series (ASSL, volume 415)

Abstract

Quiescent solar prominences are highly dynamic structures which, among other features, display oscillatory motions. The presence of these oscillations has been confirmed by means of ground- and space-based observations, and they have been classified in small and large amplitude oscillations. Since prominences are magnetized structures, the theoretical interpretation of their oscillations has been mostly done in terms of magnetohydrodynamic (MHD) waves. This interpretation has allowed the development of prominence seismology as a tool to determine prominence physical parameters (magnetic field, Alfvén speed, inhomogeneity scale, etc.) which are difficult to measure by direct means.

Keywords

Magnetic Field Strength Flux Rope Magnetic Flux Tube Small Amplitude Oscillation Magnetoacoustic Wave 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Notes

Acknowledgements

This chapter is dedicated to the memory of Josip Kleczek who woke up my interest for solar prominences.

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© Springer International Publishing Switzerland 2015

Authors and Affiliations

  1. 1.Departament de FísicaUniversitat de les Illes BalearsPalma de MallorcaSpain

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