Abstract
Results from ground based observations of low degree solar luminosity variations are presented. By using data from up to 15 consecutive excellent days the majority of the 1=0, 1 and 2 peaks in the region 2.5-3.5 mHz may marginally be identified.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Claverie, A., Isaak, G. R. and McLeod, C. P.; 1981, Solar Phys. 74, 73.
Deubner, F.-L.; 1981, Nature 290, 682.
Fröhlich, C.; 1984, Mem. S. A. It. 55, 237.
Jimenéz, A., Pallé, P. L., Perez Hernandez, F., Regulo, C., Roca Cortés, T., Domingo, V. and Korzennik, S.; these proceedings.
Woodard, M. and Hudson, H.S.: 1983. Nature 305, 589.
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
Andersen, B.N., Domingo, V. (1988). Ground 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_13
Download citation
DOI: https://doi.org/10.1007/978-94-009-4009-3_13
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-2615-5
Online ISBN: 978-94-009-4009-3
eBook Packages: Springer Book Archive