Author/Authors :
Blevis، نويسنده , , I and Boger، نويسنده , , J and Bonvin، نويسنده , , E and Cleveland، نويسنده , , B.T and Dai، نويسنده , , X and Dalnoki-Veress، نويسنده , , F and Doucas، نويسنده , , G and Farine، نويسنده , , J and Fergani، نويسنده , , H and Grant، نويسنده , , D and Hahn، نويسنده , , R.L and Hamer، نويسنده , , A.S and Hargrove، نويسنده , , C.K and Heron، نويسنده , , H and Jagam، نويسنده , , P and Jelley، نويسنده , , N.A and Jillings، نويسنده , , C and K، نويسنده ,
Abstract :
The technique used at the Sudbury Neutrino Observatory (SNO) to measure the concentration of 222Rn in water is described. Water from the SNO detector is passed through a vacuum degasser (in the light water system) or a membrane contact degasser (in the heavy water system) where dissolved gases, including radon, are liberated. The degasser is connected to a vacuum system which collects the radon on a cold trap and removes most other gases, such as water vapor and N2. After roughly 0.5 tonnes of H2O or 6 tonnes of D2O have been sampled, the accumulated radon is transferred to a Lucas cell. The cell is mounted on a photomultiplier tube which detects the α-particles from the decay of 222Rn and its progeny. The overall degassing and concentration efficiency is about 38% and the single-α counting efficiency is approximately 75%. The sensitivity of the radon assay system for D2O is equivalent to ∼3×10−15 g U/g water. The radon concentration in both the H2O and D2O is sufficiently low that the rate of background events from U-chain elements is a small fraction of the interaction rate of solar neutrinos by the neutral current reaction.
Keywords :
SnO , Radioactivity assay , RADON , Solar neutrino