Add to ORKGThe Sudbury Neutrino Observatory is a second-generation water Cherenkov detector designed to determine whether the currently observed solar neutrino deficit is a result of neutrino oscillations. The detector is unique in its use of D2O as a detection medium, permitting it to make a solar model-independent test of the neutrino oscillation hypothesis by comparison of the charged- and neutral-current interaction rates. In this paper the physical properties, construction, and preliminary operation of the Sudbury Neutrino Observatory are described. Data and predicted operating parameters are provided whenever possible
The Sudbury Neutrino Observatory (SNO) is a large-volume heavy water Cerenkov detector designed to r...
The Sudbury Neutrino Observatory (SNO) is a 1000 tonne heavy water Cherenkov detector placed 2 km un...
The Sudbury Neutrino Observatory is a 1000 T D2O Cerenkov detector that is sensitive to 8B solar neu...
The Sudbury Neutrino Observatory (SNO) is a water Cherenkov de-tector for solar neutrinos that uses ...
The Sudbury Neutrino Observatory (SNO) is a second generation solar neutrino detector. SNO is the fi...
With its heavy water target, the Sudbury Neutrino Observatory has the unique opportunity to measure ...
A method of analyzing solar neutrino measurements using water-based Cherenkov detectors is presented...
The Sudbury Neutrino Observatory uses 1000 tonnes of heavy water in an ultra-clean Cherenkov detecto...
A report is given on the status of the Sudbury Neutrino Observatory, presently under construction in...
The Sudbury Neutrino Observatory (SNO) was a water Cherenkov detector dedicated to investigate eleme...
The Sudbury Neutrino Observatory (SNO) is a water imaging Cherenkov detector. Its usage of 1000 metr...
With its heavy water target, the Sudbury Neutrino Observatory (SNO) offers the unique opportunity to...
The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cherenkov detector. Its usage of ...
The Sudbury Neutrino Observatory (SNO) was a heavy water Cerenkov detector that had the unique abili...
The Sudbury Neutrino Observatory (SNO) is a heavy-water Cherenkov detector designed to study 8B neut...
The Sudbury Neutrino Observatory (SNO) is a large-volume heavy water Cerenkov detector designed to r...
The Sudbury Neutrino Observatory (SNO) is a 1000 tonne heavy water Cherenkov detector placed 2 km un...
The Sudbury Neutrino Observatory is a 1000 T D2O Cerenkov detector that is sensitive to 8B solar neu...
The Sudbury Neutrino Observatory (SNO) is a water Cherenkov de-tector for solar neutrinos that uses ...
The Sudbury Neutrino Observatory (SNO) is a second generation solar neutrino detector. SNO is the fi...
With its heavy water target, the Sudbury Neutrino Observatory has the unique opportunity to measure ...
A method of analyzing solar neutrino measurements using water-based Cherenkov detectors is presented...
The Sudbury Neutrino Observatory uses 1000 tonnes of heavy water in an ultra-clean Cherenkov detecto...
A report is given on the status of the Sudbury Neutrino Observatory, presently under construction in...
The Sudbury Neutrino Observatory (SNO) was a water Cherenkov detector dedicated to investigate eleme...
The Sudbury Neutrino Observatory (SNO) is a water imaging Cherenkov detector. Its usage of 1000 metr...
With its heavy water target, the Sudbury Neutrino Observatory (SNO) offers the unique opportunity to...
The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cherenkov detector. Its usage of ...
The Sudbury Neutrino Observatory (SNO) was a heavy water Cerenkov detector that had the unique abili...
The Sudbury Neutrino Observatory (SNO) is a heavy-water Cherenkov detector designed to study 8B neut...
The Sudbury Neutrino Observatory (SNO) is a large-volume heavy water Cerenkov detector designed to r...
The Sudbury Neutrino Observatory (SNO) is a 1000 tonne heavy water Cherenkov detector placed 2 km un...
The Sudbury Neutrino Observatory is a 1000 T D2O Cerenkov detector that is sensitive to 8B solar neu...