Add to ORKGThe Sudbury Neutrino Observatory (SNO) was a heavy water Cerenkov detector that had the unique ability to measure both the total il active flux of solar neutrino, using a neutral current (NC) interaction, and the flux of electron neutrinos, using a charged current (CC) interaction. The experiment has demonstrated that neutrinos 3 change flavour and that the total neutrino flux is consistent with the prediction of solar models.EThOS - Electronic Theses Online ServiceGBUnited Kingdo
The solar neutrino problem arose when the first measurements of the flux of neutrinos from the Sun, ...
The Sudbury Neutrino Observatory (SNO) is a 1000 tonne heavy water Cherenkov detector placed 2 km un...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
The Sudbury Neutrino Observatory (SNO) is a second generation solar neutrino detector. SNO is the fi...
The Sudbury Neutrino Observatory (SNO) is a water Cerenkov detector designed to study solar neutrino...
The Sudbury Neutrino Observatory (SNO) is a water Cerenkov detector designed to study solar neutrino...
The Sudbury Neutrino Observatory uses 1000 tonnes of heavy water in an ultra-clean Cherenkov detecto...
The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cherenkov detector. Its usage of ...
The Sudbury Neutrino Observatory (SNO) is a water imaging Cherenkov detector. Its usage of 1000 metr...
This work presents experimental measurements obtained by analyzing the first 254 live days of data f...
The Sudbury Neutrino Observatory (SNO) is a water Cherenkov de-tector for solar neutrinos that uses ...
The Sudbury Neutrino Observatory (SNO) was a water Cherenkov detector dedicated to investigate eleme...
The Sudbury Neutrino Observatory (SNO) is a heavy-water Cherenkov detector designed to study 8B neut...
The Sudbury Neutrino Observatory (SNO) used an array of 3He proportional counters to measure the rat...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
The solar neutrino problem arose when the first measurements of the flux of neutrinos from the Sun, ...
The Sudbury Neutrino Observatory (SNO) is a 1000 tonne heavy water Cherenkov detector placed 2 km un...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
The Sudbury Neutrino Observatory (SNO) is a second generation solar neutrino detector. SNO is the fi...
The Sudbury Neutrino Observatory (SNO) is a water Cerenkov detector designed to study solar neutrino...
The Sudbury Neutrino Observatory (SNO) is a water Cerenkov detector designed to study solar neutrino...
The Sudbury Neutrino Observatory uses 1000 tonnes of heavy water in an ultra-clean Cherenkov detecto...
The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cherenkov detector. Its usage of ...
The Sudbury Neutrino Observatory (SNO) is a water imaging Cherenkov detector. Its usage of 1000 metr...
This work presents experimental measurements obtained by analyzing the first 254 live days of data f...
The Sudbury Neutrino Observatory (SNO) is a water Cherenkov de-tector for solar neutrinos that uses ...
The Sudbury Neutrino Observatory (SNO) was a water Cherenkov detector dedicated to investigate eleme...
The Sudbury Neutrino Observatory (SNO) is a heavy-water Cherenkov detector designed to study 8B neut...
The Sudbury Neutrino Observatory (SNO) used an array of 3He proportional counters to measure the rat...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...
The solar neutrino problem arose when the first measurements of the flux of neutrinos from the Sun, ...
The Sudbury Neutrino Observatory (SNO) is a 1000 tonne heavy water Cherenkov detector placed 2 km un...
The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rat...