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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, UK, in collaboration with Sheffield Hallam University, UK. They are funded by the Science and Technology Facilities Council (STFC).

BiSON operates automated resonant scattering spectrometers in astronomical domes or mirror fed systems. The current sites are:

Mount Wilson Observatory, California, USA

Las Campanas Observatory, Region IV, Chile

Observatorio del Teide, Tenerife, Canary Islands, Spain

South African Astronomical Observatory, Sutherland, South Africa

OTC Earth Station Carnarvon, Carnarvon, Western Australia

Paul Wild Observatory, Narrabri, New South Wales, Australia

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.

External links

BiSON homepage

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This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article Birmingham Solar Oscillations Network


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