Birmingham Solar Oscillations Network
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. The Birmingham Solar Oscillations Network 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. The BiSON has been collecting data continuously on solar oscillat...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. The Birmingham Solar Oscillations Network 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. 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.
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