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Time variations of the frequencies of low-degree solar p-modes

Published online by Cambridge University Press:  03 August 2017

Martin F. Woodard  and
Robert W. Noyes
Martin F. Woodard
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA
Robert W. Noyes
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA

Abstract

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A comparison of three separate years (1980, 1984, 1985) of SMM/ACRIM solar total irradiance data reveals small but significant changes in the frequencies of low-degree solar p-modes. Specifically, a decrease in the mean frequency of the nine strongest ℓ = 0 and 1 oscillation peaks was observed between 1980 and 1984 such that

Information

Type
Chapter 3: Longterm Variations in the Sun
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 197 - 200
Copyright
Copyright © Reidel 1988 

References

1. Woodard, M. F., and Noyes, R. W., Nature 318, 449–450 (1985).Google Scholar
2. Grec, G., Fossat, E. and Pomerantz, M., Sol. Phys. 82. 55–66 (1983).Google Scholar