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Touching on the Effects of an Imperfect Window Function

Published online by Cambridge University Press:  08 February 2017

W.J. Chaplin
Affiliation:
School of Physics & Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT UK, E-mail: wjc@star.sr.bham.ac.uk
Y. Elsworth
Affiliation:
School of Physics & Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT UK, E-mail: wjc@star.sr.bham.ac.uk
G.R. Isaak
Affiliation:
School of Physics & Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT UK, E-mail: wjc@star.sr.bham.ac.uk
C.P. McLeod
Affiliation:
School of Physics & Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT UK, E-mail: wjc@star.sr.bham.ac.uk
B.A. Miller
Affiliation:
School of Physics & Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT UK, E-mail: wjc@star.sr.bham.ac.uk
R. New
Affiliation:
School of Science & Mathematics, Sheffield Hallam University, Sheffield, S1 1WB

Extract

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BiSON currently consists of four fully- and two semi-automated observatories, dedicated to the round-the-clock collection of low-degree (low-l) helioseismological data. A complete historical record of the network can be found in Chaplin et al. (1996). The annual duty cycles achieved by BiSON have improved steadily since our sixth site was commissioned in 1992. Over the period 1992 – 1996 inclusive, we have recorded annual duty cycles of: 54. 68. 78. 74 and 78 per cent respectively.

Type
I. Global Structure and Evolution of the Solar and Stellar Interior
Copyright
Copyright © Kluwer 1998 

References

Chaplin, W. J., Elsworth, Y., Howe, R., Isaak, G. R., McLeod, C. P., Miller, B. A., New, R., van der Raay, H. B. and Wheeler, S. J., Solar Physics, 1996, 168, 1 Google Scholar
Chaplin, W. J., Elsworth, Y., Howe, R., Isaak, G. R., McLeod, C. P., Miller, B. A. and New, R., 1997, MNRAS, 1997, 287, 51 Google Scholar