Birmingham Solar Oscillations Network

From Wikipedia, the free encyclopedia

The Birmingham Solar Oscillations Network stations.  The distribution in longitude allows for near-continuous observations of the Sun.
The Birmingham Solar Oscillations Network stations. The distribution in longitude allows for near-continuous observations of the Sun.

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 Particle Physics and Astronomy Research Council (PPARC).

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

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.

[edit] External links