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Observational aspects of prominence oscillations

Published online by Cambridge University Press:  01 September 2007

Oddbjørn Engvold
Oddbjørn Engvold*
Affiliation:
Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029, Blindern, N-0315 Oslo, Norway email: oengvold@astro.uio.no
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Abstract

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Seismology has become a powerful tool in studies of the magnetic structure of solar prominences and filaments. Reversely, analytical and numerical models are guided by available information about the spatial and thermodynamical structure of these enigmatic structures. The present invited paper reviews recent observational results on oscillations and waves as well as details about small-scale structures and dynamics of prominences and filaments.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S247: Waves & Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology , September 2007 , pp. 152 - 157
Copyright
Copyright © International Astronomical Union 2008

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