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


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.


Sunspot Group Solar Limb Doppler Width Quiescent Prominence Noise Storm 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.


  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

Personalised recommendations