Home
Home
Neutrino's
Cosmic Rays
Reactions
Results
References

Sudbury Neutrino Observatory

The Sudbury Neutrino Observatory (SNO) is taking data that will explain the properties of neutrinos and the core of the sun.

The detector  was built 6800 feet under ground, in INCO's Creighton mine near Sudbury, Ontario. SNO is a heavy-water Cherenkov detector that is designed to detect neutrinos produced by fusion reactions in the sun.

It uses 1000 tonnes of heavy water contained in a 12 meter diameter acrylic vessel. Neutrino's react with the heavy water (D2O) to produce flashes of light called Cherenkov radiation.

This light is then detected by an array of 10,000 photomultiplier tubes mounted on a geodesic support structure surrounding the heavy water vessel.

The detector is immersed in light (normal) water within a 30 meter barrel-shaped cavity (the size of a 10 story building!) excavated from Norite rock.

Located in the deepest part of the mine, the rock shields the detector from majority of the cosmic rays, and allows you to only view reactions caused by the more powerful rays, ie the ones from our sun. The detector laboratory is extremely clean to reduce background signals from radioactive elements present in the mine dust which would otherwise hide the very weak signal from neutrino's.

Do you want to

How much do you know about the Sudbury Neutrino Observatory?

learn more about SNO?

Click the Navigation Bar to explore the detector, and to find out how it works.

Website Developed for Radiation Detection and Measurement, Physics 391

[Home] [Neutrino's] [Cosmic Rays] [Reactions] [Results] [References]

Andrea T. Hughes - March 2004