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Earth Based Observations of Solar Luminosity Oscillations

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Advances in Helio- and Asteroseismology

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.

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References

  1. Woodard M. and Hudson H., Nature, 305, 589–593, (1983)

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  2. Claverie, A., Isaak, G.R., McLeod, C.P., van der Raay, H.B. and Roca Cortes, T., 1979 Nature, 22, 591–594.

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  3. Domingo V. et al. In preparation

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  4. Jiménez, A., Pallé, P.L., Roca Cortés, T., Domingo, V., Korzennik, S.: 1986, Astron. & Astroph., (in press)

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© 1988 International Astronomical Union

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Jiménez, A. et al. (1988). Earth Based Observations of Solar Luminosity Oscillations. In: Christensen-Dalsgaard, J., Frandsen, S. (eds) Advances in Helio- and Asteroseismology. International Astronomical Union / Union Astronomique Internationale, vol 123. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4009-3_14

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  • DOI: https://doi.org/10.1007/978-94-009-4009-3_14

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-277-2615-5

  • Online ISBN: 978-94-009-4009-3

  • eBook Packages: Springer Book Archive

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