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A Contribution to the Understanding of Chromospheric Oscillations

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Abstract

We present SUMER/SOHO UV measurements of chromospheric oscillations of intensity, velocity, and linewidth observed in C i, S i, O i, and C ii lines, which are formed in the altitude range from 1000 km to 2000 km above τ 500=1. Oscillations in lines originating at similar altitudes exhibit different behaviors which we discuss in terms of the formation of the lines.

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Authors and Affiliations

  1. Institut d’Astrophysique Spatiale (IAS), Bât. 121, CNRS (UMR 8617) and Université Paris-Sud 11, 91405, Orsay, France

    F. Baudin, J.-C. Vial, K. Bocchialini & P. Lemaire

  2. Instituto de Astronomía y Física del Espacio, CONICET, 1428, Buenos Aires, Argentina

    E. Ibarra, A. Costa & M. Rovira

  3. Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA, 02138, USA

    E. H. Avrett

Authors
  1. F. Baudin
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  2. E. Ibarra
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  3. E. H. Avrett
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  4. J.-C. Vial
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  5. K. Bocchialini
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  6. A. Costa
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  7. P. Lemaire
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  8. M. Rovira
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Correspondence to F. Baudin.

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Baudin, F., Ibarra, E., Avrett, E.H. et al. A Contribution to the Understanding of Chromospheric Oscillations. Sol Phys 241, 39–51 (2007). https://doi.org/10.1007/s11207-007-0006-3

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  • DOI: https://doi.org/10.1007/s11207-007-0006-3

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