Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-25T05:19:58.622Z Has data issue: false hasContentIssue false
  • English
  • Français

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]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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 

References

Arregui, I., Terradas, J., Oliver, R., & Ballester, J. L. 2008, ApJ (Letters), 682, L141CrossRefGoogle Scholar
Arregui, I. & Asensio Ramos, A. 2011, ApJ (Letters), 740, 44CrossRefGoogle Scholar
Arregui, I., Oliver, R., & Ballester, J. L. 2012, Living Reviews in Solar Physics, 9, 2CrossRefGoogle Scholar
Arregui, I., Asensio Ramos, A., & Pascoe, D. J. 2013, ApJ, 769, L34CrossRefGoogle Scholar
Díaz, A. J., Oliver, R., & Ballester, J. L. 2002, ApJ, 580, 550CrossRefGoogle Scholar
Dymova, M. V. & Ruderman, M. S. 2005, Solar Phys., 229, 79Google Scholar
Engvold, O. 1998, in Webb, D. F., Schmieder, B., & Rust, D. M. (eds.) New Perspectives in Solar Prominences, Proc. IAU Colloq. No. 167 (San Francisco, ASP), p. 23Google Scholar
Engvold, O. 2008, in Erdélyi, R., & Mendoza-Briceño, C. A. (eds.) Waves & Oscillations in the Solar Atmosphere, Proc. IAU Symp. No. 247 (San Francisco, ASP), p. 152Google Scholar
Goossens, M., Arregui, I., Ballester, J. L., & Wang, T. J. 2008, A & A, 484, 851CrossRefGoogle Scholar
Hyder, C. L. 1966, ZfA, 63, 78Google Scholar
Isobe, H. & Tripathi, D. 2006, A & A, 449, L17Google Scholar
Jing, J., Lee, J., Spirock, T. J., Xu, Y., Wang, H., & Choe, G. S. 2003, ApJ (Letters), 584, L103CrossRefGoogle Scholar
Jing, J., Lee, J., & Spirock, T. J., Wang, H. 2006, Solar Phys., 236, 97Google Scholar
Joarder, P. & Roberts, B. 1993, A & A, 277, 225Google Scholar
Kleczek, J. & Kuperus, M. 1969, Solar Phys., 6, 72CrossRefGoogle Scholar
Lin, Y. 2004, Ph.D. Thesis, University of Oslo, NorwayGoogle Scholar
Lin, Y., Engvold, O., Rouppe Van der Voort, L. H. M., Wiik, J. E., & Berger, T. E. 2005, Solar Phys., 225, 229Google Scholar
Lin, Y., Engvold, O., Rouppe Van der Voort, L. H. M., & Van Noort, M. J. 2007, Solar Phys., 246, 65CrossRefGoogle Scholar
Lin, Y., Martin, S. F., Engvold, O., Rouppe Van der Voort, L. H. M., & Van Noort, M. J. 2003, Adv. Sp. Res., 42, 803CrossRefGoogle Scholar
Lin, Y., Soler, R., Engvold, O., Ballester, J. L., Langagen, O., Oliver, R. & Rouppe Van der Voort, L. H. M. 2009, ApJ, 704, 870CrossRefGoogle Scholar
Luna, M. & Karpen, J. 2012, ApJ (Letters), 750, L1CrossRefGoogle Scholar
Luna, M., Díaz, A. J., & Karpen, J. 2012, ApJ (Letters), 757, L98Google Scholar
Okamoto, T. J., Tsuneta, S., Berger, T. E., Ichimoto, K., Katsukawa, Y., Lites, B. W., Nagata, S., Shibata, K, Shimizu, T., Shine, R. A., Suematsu, Y., Tarbell, T. D., & Title, A. M. 2007, Science, 318, 1577Google Scholar
Pintér, B., Jain, R., Tripathi, D., & Isobe, H. 2008, ApJ 680, 1560CrossRefGoogle Scholar
Pouget, G., Bocchialini, K., & Solomon, J. 2006, A & A 450, 1189Google Scholar
Ramsey, H. E. & Smith, S. F. 1966, AJ, 71, 197Google Scholar
Régnier, S., Solomon, J., & Vial, J. C. 2001, A & A, 376, 292CrossRefGoogle Scholar
Roberts, B. & Joarder, P. 1994, in Belvedere, G., Rodon, M., & Simnett, G. M. (eds.) Advances in Solar Physics, Proc. seventh European Meeting on Solar Physics (Lecture Notes in Physics 432, Springer), p. 173ARAA, 41, 241Google Scholar
Roberts, B., Edwin, P. M., & Benz, A. O. 1984, ApJ, 279, 857Google Scholar
Rosenberg, H. 1970, A & A, 9, 159Google Scholar
Ruderman, M. & Goossens, M. 2013, Solar Phys. (In press)Google Scholar
Soler, R., Arregui, I., Oliver, R., & Ballester, J. L. 2010, ApJ, 722, 1778CrossRefGoogle Scholar
Terradas, J., Arregui, I., Oliver, R., & Ballester, J. L. 2008, ApJ (Letters), 978, L153CrossRefGoogle Scholar
Tripathi, D., Isobe, H., & Jain, R. 2009, Space Sci. Revs, 149, 283Google Scholar
Uchida, Y. 2004, PASJ, 22, 341Google Scholar
Vial, J. C. 1998, in Webb, D. F., Schmieder, B., & Rust, D. M. (eds.) New Perspectives in Solar Prominences, Proc. IAU Colloq. No. 167 (San Francisco, ASP), p. 175Google Scholar
Vršnak, B., Veronig, A. M., Thalman, J. K. & Žic, T. 2007, ApJ, 647, 676Google Scholar
Zhang, Q. M., Chen, P. F., Xia, C., Keppens, R., & Ji, H. S. 2013, A & A, 554, A124Google Scholar