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SNO  Sudbury Neutrino Observatory

The Sudbury Neutrino Observatory (SNO) is taking data that will provide revolutionary insight into the properties of neutrinos and the core of the sun. The detector, shown in the artist's conception below, was built 6800 feet below ground, in INCO's Creighton mine near Sudbury, Ontario. SNO is designed to detect neutrinos produced by fusion reactions in the sun. SNO is a heavy-water Cherenkov detector. It uses 1000 tonnes of heavy water, on loan from Atomic Energy of Canada Limited (AECL), contained in a 12m diameter acrylic vessel. Neutrinos react with the heavy water (D2O) to produce flashes of light called Cherenkov radiation. This light is then detected with a geodesic array of 9600 photomultiplier tubes surrounding the heavy water vessel. The detector is immersed in light (normal) water within a 30m barrel-shaped cavity excavated from Norite rock. Location in the deepest part of the mine provides an overburden of rock to shield from cosmic rays. The detector laboratory is immensely clean to reduce background radiation signals which would otherwise hide the very weak signal from neutrinos.

Artist Conception