Height-Dependent Short-Period Oscillations in the Fe XIV (530.3 nm) Solar Corona Above a Sunspot Group Crossing the Limb

  • V. N. Dermendjiev
Conference paper

Abstract

A sequence of 86 green coronal line spectra is analyzed in order to find short-period oscillations in the corona. It is shown that a tendency exists of the revealed periods to change with the height above the limb.

Keywords

Boulder 

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References

  1. Dermendjiev, V.N., Rybansky, M., Rusin, V., Buyukliev, G.T., Zlateva, E.B.: 1986, Contr. Astron. Obs. Skalnate Pleso 15, 429.ADSGoogle Scholar
  2. Haykin, S.: 1983 in “Nonlinear Methods of Spectral Analysis” ed. Haykin S., Springer-Verlag.CrossRefGoogle Scholar
  3. Koutchmy S.: 1981, Space Sci. Rev. 29, 375.ADSCrossRefGoogle Scholar
  4. Minarovjech, M., Rusin, V., Rybansky, M.: 1983, Publ. of Debrecen Heliophys. Obs. 5, 511.ADSGoogle Scholar
  5. Tsubaki, T.: 1977, Solar Phys. 51, 121.ADSCrossRefGoogle Scholar
  6. Tsubaki, T.: 1988, in “Solar and stellar coronal structures and dynamics”, ed. R. C. Altrock, Proc. 9th Sac. Peak Summer Symp., Sunspot, NM, 17–21 Aug 1987, 140.Google Scholar

Copyright information

© Springer-Verlag Berlin Heidelberg 1991

Authors and Affiliations

  • V. N. Dermendjiev
    • 1
  1. 1.Department of Astronomy and NAOSofiaBulgaria

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