Astronomy:Birmingham Solar Oscillations Network

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Short description: Network of six solar helioseismology observatories

Birmingham Solar Oscillations Network

The Birmingham Solar Oscillations Network (BiSON) consists of a network of six remote solar observatories monitoring low-degree solar oscillation modes. It is operated by the High Resolution Optical Spectroscopy group of the School of Physics and Astronomy at the University of Birmingham, United Kingdom , in collaboration with Sheffield Hallam University, United Kingdom . They are funded by the Science and Technology Facilities Council (STFC).[1]

The BiSON has been collecting data continuously on solar oscillations since 1976, making it the longest running helioseismology network with data covering three solar cycles.[2]

Team

Academic staff

  • Professor Yvonne Elsworth (Head of project)
  • Professor Bill Chaplin

Research staff

Technical staff

  • Mr Ian Barnes — Electronics
  • Mr Barry Jackson — Mechanics

Remote observatories

The BiSON stations. The distribution in longitude allows for near-continuous observations of the Sun.

BiSON operates automated resonant scattering spectrometers in astronomical domes or mirror fed systems. The network was established in 1976 with two permanent stations; the addition of several more sites culminated with the addition of a sixth in 1992.[3] The current sites are:

See also

References

  1. "BiSON :: Home". http://bison.ph.bham.ac.uk/. Retrieved 16 May 2009. 
  2. "BiSON The Birmingham Solar-Oscillations Network". Archived from the original on 11 June 2007. https://web.archive.org/web/20070611210739/http://astro.phys.au.dk/SONG/WORKSHOP-2006/Miller.ppt. Retrieved 16 May 2009. 
  3. Chaplin, W. J.; Elsworth, Y.; Isaak, G. R.; McLeod, C. P.; Miller, B. A.; New, R. (May 1996). "Recent Results from the Birmingham Solar-Oscillations Network (BiSON)". American Astronomical Society 188 (1996AAS...188.6904C): 936. Bibcode1996AAS...188.6904C. 

External links