Advertisement

Earth Based Observations of Solar Luminosity Oscillations

  • A. Jiménez
  • P. L. Pallé
  • F. Pérez Hernández
  • C. Régulo
  • T. Roca Cortés
  • V. Domingo
  • S. Korzennik
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 123)

Abstract

Earth based multichannel photometry of integral sunlight has been obtained at Izafia (Tenerife) during 1984–1986. Power spectra of the solar luminosity variations of individual days show power in the 5 minute interval above noise at a level comparable to SMM data(1). When combining contigous days of data the signature of p mode solar oscillations spectrum appears, although individual peak identification is difficult.

Keywords

Power Spectrum Solar Intensity Average Power Spectrum Solar Maximum Mission Solar Luminosity 
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.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. (1).
    Woodard M. and Hudson H., Nature, 305, 589–593, (1983)ADSCrossRefGoogle Scholar
  2. (2).
    Claverie, A., Isaak, G.R., McLeod, C.P., van der Raay, H.B. and Roca Cortes, T., 1979 Nature, 22, 591–594.ADSCrossRefGoogle Scholar
  3. (3).
    Domingo V. et al. In preparationGoogle Scholar
  4. (4).
    Jiménez, A., Pallé, P.L., Roca Cortés, T., Domingo, V., Korzennik, S.: 1986, Astron. & Astroph., (in press)Google Scholar

Copyright information

© International Astronomical Union 1988

Authors and Affiliations

  • A. Jiménez
    • 1
  • P. L. Pallé
    • 1
  • F. Pérez Hernández
    • 1
  • C. Régulo
    • 1
  • T. Roca Cortés
    • 1
  • V. Domingo
    • 2
  • S. Korzennik
    • 2
  1. 1.Instituto de Astrofisica de CanariasUniversidad de La LagunaTenerifeSpain
  2. 2.Space Science Department for ESA. ESTECNoordwijkNetherlands

Personalised recommendations