Abstract
Prominence seismology is a rapidly developing topic which seeks to infer the internal structure and properties of solar prominences from the study of its oscillations. Two-dimensional high-resolution observations suggest that filaments can be considered as made by small scale fibrils, having a cool region, stacked one after another in the vertical and horizontal directions. An extense observational background about oscillations in filaments has been gathered during the last 20 years and these observations point out that fibrils or groups of fibrils can oscillate independently. From the theoretical point of view, small amplitude oscillations in single and multifibril configurations have been studied as a first step to explain observational features.
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Ballester, J. L.: 2003, In R. Erdélyi, K. Petrovay, B. Roberts and M. Aschwanden (eds.), Turbulence, Waves and Instabilities in the Solar Plasma. Springer, Dordrecht, 193–213.
Ballester, J. L.: 2006, Phil. Trans. R. Soc. A 364, 405–415.
Díaz, A. J., Oliver, R., Erdélyi, R., and Ballester, J. L.: 2001, Astron. Astrophys. 379, 1083–1097.
Díaz, A. J., Oliver, R., and Ballester, J. L.: 2002, Astrophys. J. 580, 550–565.
Díaz, A. J., Oliver, R., and Ballester, J. L.: 2003, Astron. Astrophys. 402, 781–789.
Díaz, A. J., Oliver, R., and Ballester, J. L.: 2005, Astron. Astrophys. 440, 1167–1175.
Dyson, F. A.: 1930, M. N., 91, 239–241.
Engvold, O.: 2001, In J. L. Ballester and B. Roberts (eds.), Proc. of Workshop on MHD Waves in Astrophysical Plasmas. Universitat de les Illes Balears, 123–131.
Engvold, O.: 2005, In A. V. Stepanov, E. E. Benevolenskaya and A. G. Kosovichev (eds.), Proc. IAU Colloq. on Multiwavelength Investigations of Solar Activity, Cambridge University Press.
Joarder, P. S., Nakariakov, V. M., and Roberts, B.: 1997, Solar Phys. 173, 81–101.
Joarder, P. S. and Roberts, B.: 1992, Astron. Astrophys. 256, 264–272.
Lin, Y.: 2005, Ph. D. Thesis, University of Oslo, Norway.
Lin, Y., Engvold, O., Van der Voort, L. R., Wiik, J. E., and Berger, T. E.: 2005, Solar Phys. 226, 239–254.
Oliver, R.: 2004, In R. Erdélyi, J. L. Ballester and B. Fleck B. sci. eds. Proc. of SOHO 13 “Waves Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE”. ESA SP-547, 175–184.
Oliver, R. and Ballester, J. L.: 2002, Solar Phys. 206, 45–67.
Wiehr, E.: 2004, In R. Erdélyi, J. L. Ballester and B. Fleck B. sci. (eds.) Proc. of SOHO 13 “Waves Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE,” ESA SP-547, 185–192.
Yi, Z. and Engvold, O.: 1991, Solar Phys. 134, 275–286.
Yi, Z., Engvold, O., and Keil, S. L.: 1991a, Solar Phys. 132, 63–80.
Zirker, J. B., Engvold, O., and Martin S. F.: 1998, Nature 396, 440.
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Ballester, J.L. Seismology of Prominence-Fine structures: Observations and Theory. Space Sci Rev 122, 129–135 (2006). https://doi.org/10.1007/s11214-006-7016-6
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DOI: https://doi.org/10.1007/s11214-006-7016-6