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Splitting of the low ℓ solar p modes

Published online by Cambridge University Press:  03 August 2017

S.M. Jefferies ,
C.P. McLeod ,
H.B. van der Raay ,
P.L. Palle  and
T. Roca Cortes
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
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
T. Roca Cortes
Affiliation:
Instituto de Astrofisica de Canarias, Universidad de la Laguna, Tenerife

Abstract

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An analysis of full disc line of sight velocity data yield line splitting values of the low ℓ-value non-radial modes. Possible variations of the line splitting with the solar cycle are investigated.

Type
Chapter 1: Observations of Solar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 25 - 28
Copyright
Copyright © Reidel 1988 

References

1. van der Raay, H.B., Palle, P.L. and Roca, T. Cortes in Seismology of the Sun and the Distant Stars. (ed. Gough, D.O., NATO ASI 169 (1985) p. 215)Google Scholar
2. van der Raay, H.B., Palle, P.L. and Roca, T. Cortes in Seismology of the Sun and Distant Stars. (ed. Gough, D.O. NATO ASI 169 (1985) p.333)Google Scholar