Birmingham Solar Oscillations Network

Birmingham Solar Oscillations Network
BiSON Las Campanas Station.jpg
BiSON telescope at Las Campanas Observatory in Atacama Region, Chile.
Alternative namesBiSON Edit this at Wikidata
OrganizationUniversity of Birmingham Edit this on Wikidata
Telescope stylesolar telescope Edit this on Wikidata
Websitebison.ph.bham.ac.uk Edit this at Wikidata
  Related media on Commons

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).

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.

Team

Academic staff

Research staff

Technical staff

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. The current sites are:

See also


This page was last updated at 2023-04-17 01:17 UTC. Update now. View original page.

All our content comes from Wikipedia and under the Creative Commons Attribution-ShareAlike License.


Top

If mathematical, chemical, physical and other formulas are not displayed correctly on this page, please useFirefox or Safari