Bison performance

CHAPLIN, W. J., ELSWORTH, Y., HOWE, R., ISAAK, G. R., MCLEOD, C. P., MILLER, B. A., VANDERRAAY, H. B., WHEELER, S. J. and NEW, R. (1996). Bison performance. Solar Physics, 168 (1), 1-18.

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Link to published version:: https://doi.org/10.1007/BF00145821
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    Abstract

    Since 1981 we have been operating the Birmingham Solar-Oscillations Network (BiSON), a global network of resonant-scattering spectrometers, observing the low-l solar p modes. Here we discuss historical developments, culminating in the establishment of a 6-station network in 1992 September, and the subsequent performance of that network. The data record of each station from 1992 to 1994 has been analysed in terms of weather and equipment breakdowns. Our early experience suggests that the best long-term coverage possible with a 6-station network is limited in practice to about 80%, which falls short of previous predictions.

    Item Type: Article
    Research Institute, Centre or Group - Does NOT include content added after October 2018: Materials and Engineering Research Institute > Thin Films Research Centre > Nanotechnology Centre for PVD Research
    Identification Number: https://doi.org/10.1007/BF00145821
    Page Range: 1-18
    Depositing User: Ann Betterton
    Date Deposited: 09 Jun 2010 15:54
    Last Modified: 18 Mar 2021 09:15
    URI: http://shura.shu.ac.uk/id/eprint/2035

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