The Sudbury Neutrino Observatory consists of a 1 kiloton heavy water Cherenkov detector able to detect and reconstruct high-energy muons created from cosmic ray showers and atmospheric neutrino interactions. By measuring the flux of through-going muons as a function of zenith angle, the SNO experime
✦ LIBER ✦
Measurement of 222Rn dissolved in water at the Sudbury Neutrino Observatory
✍ Scribed by I Blevis; J Boger; E Bonvin; B.T Cleveland; X Dai; F Dalnoki-Veress; G Doucas; J Farine; H Fergani; D Grant; R.L Hahn; A.S Hamer; C.K Hargrove; H Heron; P Jagam; N.A Jelley; C Jillings; A.B Knox; H.W Lee; I Levine; M Liu; S Majerus; A McDonald; K McFarlane; C Mifflin; A.J Noble; S Noël; V.M Novikov; J.K Rowley; M Shatkay; J.J Simpson; D Sinclair; B Sur; J.-X Wang; M Yeh; X Zhu
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 385 KB
- Volume
- 517
- Category
- Article
- ISSN
- 0168-9002
No coin nor oath required. For personal study only.
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