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Solar cycle dependence of solar p nodes

Published online by Cambridge University Press:  03 August 2017

G.R. Isaak ,
S.M. Jefferies ,
C.P. Mcleod ,
R. New ,
H.B. van der Raay ,
P.L. Palle ,
C. Regulo  and
T. Roca Cortes
G.R. Isaak
Affiliation:
Department of Physics, University of Birmingham, Birmingham B15 2TT, England
S.M. Jefferies
Affiliation:
Department of Physics, University of Birmingham, Birmingham B15 2TT, England
C.P. Mcleod
Affiliation:
Department of Physics, University of Birmingham, Birmingham B15 2TT, England
R. New
Affiliation:
Department of Physics, University of Birmingham, Birmingham B15 2TT, England
H.B. van der Raay
Affiliation:
Department of Physics, University of Birmingham, Birmingham B15 2TT, England
P.L. Palle
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de la Laguna, Tenerife
C. Regulo
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de la Laguna, Tenerife
T. Roca Cortes
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de la Laguna, Tenerife

Abstract

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Data obtained at Izana (Tenerife) and Haleakala (Maui), using optical resonant scattering with a potassium vapour cell over the years 1980–84, are used to determine the frequencies of the low ℓ p modes. Possible variation in these frequencies with the solar cycle are investigated.

Type
Chapter 3: Longterm Variations in the Sun
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 201 - 204
Copyright
Copyright © Reidel 1988 

References

1. van der Raay, H.B. in Theoretical Problems in Stellar Stability ana Oscillations 215–219 (University of Liege 1984)Google Scholar
2. Woodard, M.F. and Noyes, R.W., Nature 318 (1985) 449–450 CrossRefGoogle Scholar