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:: 10.1007/BF00145821

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: Materials and Engineering Research Institute > Thin Films Research Centre > Nanotechnology Centre for PVD Research
Identification Number: 10.1007/BF00145821
Depositing User: Ann Betterton
Date Deposited: 09 Jun 2010 16:54
Last Modified: 09 Jun 2010 16:54
URI: http://shura.shu.ac.uk/id/eprint/2035

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