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1 results

  • Prominence Seismology

  • J. L. Ballester
  • Journal:
    Proceedings of the International Astronomical Union / Volume 8 / Issue S300 / June 2013
    Published online by Cambridge University Press:
    06 January 2014, pp. 30-39
    Print publication:
    June 2013
    • Article
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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.