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Dynamics of a Quiescent Solar Prominence Observed with the SUMER/SOHO Instrument

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Abstract

We present the results obtained from analyzing SUMER/SOHO observational data of a quiescent solar prominence. The studied prominence is made of complex structures. From the 1-hr data set, we derive characteristic frequencies in terms of intensity and velocity oscillations, as measured in 4 transition-region lines. The presence of different types of frequencies is detected: chromospheric oscillations and intermediate periods (6 min to 12 min). This result suggests that these oscillations are transmitted by the magnetic fields from the chromosphere to the transition region.

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Authors and Affiliations

  1. Institut d'Astrophysique Spatiale, Université Paris XI - CNRS, Bâtiment 121, 91405, Orsay Cedex, France

    K. Bocchialini & J.C. Vial

  2. Instituto de Astronomí a y Fí sica del Espacio CC 67, Suc. 28, 1428, Buenos Aires, Argentina

    A. Costa, G. Domenech, M. Rovira & K. Wingfield

Authors
  1. K. Bocchialini
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  2. A. Costa
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  3. G. Domenech
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  4. M. Rovira
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  5. J.C. Vial
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  6. K. Wingfield
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Bocchialini, K., Costa, A., Domenech, G. et al. Dynamics of a Quiescent Solar Prominence Observed with the SUMER/SOHO Instrument. Solar Physics 199, 133–143 (2001). https://doi.org/10.1023/A:1010395012130

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  • DOI: https://doi.org/10.1023/A:1010395012130

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