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Four methods for determining the composition of low-level uranium- and thorium-chain surface contamination are presented.
Direct approach to resolve the solar-neutrino problem
H. H. Chen · 1985
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The Use of Photomultipliers in SNO
R. K. Taplin · 1995
Earlier work this paper cites.
Table of Isotopes
R. B. Firestone, V. S. Shirley, C. M. Baglin, S. Y. F. Chu, and J. Zipkin · 1996
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3 He Neutral Current Detectors for the Sudbury Neutrino Observatory
P. M. Thornewell · 1997
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The Sudbury Neutrino Observatory
SNO Collaboration · 2000
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Radiation Detection and Measurement
G. F. Knoll · 2000
Cited alongside, same era.
Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory
Q. R. Ahmad et al · 2002
Cited alongside, same era.
A radium assay technique using hydrous titanium oxide adsorbent for the Sudbury Neutrino Observatory
T. C. Andersen et al · 2003
Cited alongside, same era.
Review of Particle Physics
W.-M. Yao et. al · 2006
Cited alongside, same era.
An array of low-background 3 He proportional counters for the Sudbury Neutrino Observatory
J. F. Amsbaugh et al · 2007
Later among the works it cites.
An Independent Measurement of the Total Active 8 B Solar Neutrino Flux Using an Array of 3 He Proportional Counters at the Sudbury Neutrino Observatory
SNO Collaboration · 2008
Later among the works it cites.
Low Energy Background in the NCD Phase of the Sudbury Neutrino Observatory
H. M. O’Keeffe · 2008
Later among the works it cites.
High sensitivity measurement of 224
B. Aharmim et al · 2009
Later among the works it cites.
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