Title of article :
Optical calibration hardware for the Sudbury Neutrino Observatory
Author/Authors :
Moffat، نويسنده , , B.A. and Ford، نويسنده , , R.J. and Duncan، نويسنده , , F.A. and Graham، نويسنده , , K. and Hallin، نويسنده , , A.L. and Hearns، نويسنده , , C.A.W. and Maneira، نويسنده , , J. and Skensved، نويسنده , , P. and Grant، نويسنده , , D.R.، نويسنده ,
Pages :
11
From page :
255
To page :
265
Abstract :
The optical properties of the Sudbury Neutrino Observatory (SNO) heavy water Cherenkov neutrino detector are measured in situ using a light diffusing sphere (“laserball”). This diffuser is connected to a pulsed nitrogen/dye laser via specially developed underwater optical fibre umbilical cables. The umbilical cables are designed to have a small bending radius, and can be easily adapted for a variety of calibration sources in SNO. The laserball is remotely manipulated to many positions in the D 2 O and H 2 O volumes, where data at six different wavelengths are acquired. These data are analysed to determine the absorption and scattering of light in the heavy water and light water, and the angular dependence of the response of the detectorʹs photomultiplier tubes. This paper gives details of the physical properties, construction, and optical characteristics of the laserball and its associated hardware.
Keywords :
Water Cherenkov detector , Pulsed optical source , Underwater umbilical cable , Photomultiplier angular response , detector calibration , Laserball , Light diffusing sphere , Sudbury Neutrino Observatory , Timing calibration of large PMT array
Journal title :
Astroparticle Physics
Record number :
2026968
Link To Document :
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