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.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Woodard M. and Hudson H., Nature, 305, 589–593, (1983)
Claverie, A., Isaak, G.R., McLeod, C.P., van der Raay, H.B. and Roca Cortes, T., 1979 Nature, 22, 591–594.
Domingo V. et al. In preparation
Jiménez, A., Pallé, P.L., Roca Cortés, T., Domingo, V., Korzennik, S.: 1986, Astron. & Astroph., (in press)
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1988 International Astronomical Union
About this paper
Cite this paper
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
Download citation
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