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Experience in operating a limited global network of stations measuring full-disc oscillations of the Sun

Published online by Cambridge University Press:  03 August 2017

Y.P. Elsworth
Affiliation:
Department of Physics, University of Birmingham, Birmingham B15 2TT, England
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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Details are given about the operation of a two station network and of a new semi-automatic station which has recently been added. Comparison is made with predicted duty cycles. A possible way of quantifying the sky quality is also given.

Type
Chapter 10: Network and Space Observations of Solar and Stellar Oscillations
Copyright
Copyright © Reidel 1988 

References

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