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Prominence Seismology

Published online by Cambridge University Press:  06 January 2014

J. L. Ballester
J. L. Ballester*
Affiliation:
Departament de Física, Universitat de les Illes Balears, E - 07122, Palma de Mallorca, Spain email: [email protected]
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Abstract

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Quiescent solar prominences are cool and dense plasma clouds located inside the hot and less dense solar corona. They are highly dynamic structures displaying flows, instabilities, oscillatory motions, etc. The oscillations have been mostly interpreted in terms of magnetohydrodynamic (MHD) waves, which has allowed to perform prominence seismology as a tool to determine prominence physical parameters difficult to measure. Here, several prominence seismology applications to large and small amplitude oscillations are reviewed.

Keywords

Prominence OscillationsMHD Waves
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 30 - 39
Copyright
Copyright © International Astronomical Union 2013 

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