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Ground based observations of solar luminosity oscillations

Published online by Cambridge University Press:  03 August 2017

B. N. Andersen  and
V. Domingo
B. N. Andersen
Affiliation:
Space Science Department of ESA, ESTEC, Noordwijk, The Netherlands
V. Domingo
Affiliation:
Space Science Department of ESA, ESTEC, Noordwijk, The Netherlands

Abstract

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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.

Type
Chapter 1: Observations of Solar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 67 - 69
Copyright
Copyright © Reidel 1988 

References

Claverie, A., Isaak, G. R. and McLeod, C. P.; 1981, Solar Phys. 74, 73.CrossRefGoogle Scholar
Deubner, F.-L.; 1981, Nature 290, 682.CrossRefGoogle Scholar
Fröhlich, C.; 1984, Mem. S. A. It. 55, 237.Google Scholar
Jimenéz, A., Pallé, P. L., Perez Hernandez, F., Regulo, C., Roca Cortès, T., Domingo, V. and Korzennik, S.; these proceedings.Google Scholar
Woodard, M. and Hudson, H.S.; 1983, Nature 305, 589.CrossRefGoogle Scholar