K. McFarlane
Carleton University
12 Papers
128 Citations
K. McFarlane is an academic researcher from Carleton University. The author has contributed to research in topics: Sudbury Neutrino Observatory & Solar neutrino. The author has an hindex of 10, co-authored 12 publications.
Chat about Author
Papers
Direct evidence for neutrino flavor transformation from neutral current interactions in the Sudbury Neutrino Observatory
Q. R. Ahmad,R. C. Allen,T. C. Andersen,J. D. Anglin,J. C. Barton,E. W. Beier,M. Bercovitch,J. Bigu,S. D. Biller,R. A. Black,I. Blevis,R. J. Boardman,J. Boger,E. Bonvin,M.G. Boulay,M.G. Boulay,M. G. Bowler,T. J. Bowles,S. J. Brice,S. J. Brice,M. C. Browne,M. C. Browne,T. V. Bullard,G. Bühler,J. Cameron,Yuen-Dat Chan,Herbert H. Chen,M. L. Chen,Xin Chen,Xin Chen,B. T. Cleveland,E. T.H. Clifford,J. H.M. Cowan,D. F. Cowen,G. A. Cox,X. Dai,F. Dalnoki-Veress,W. F. Davidson,P. J. Doe,P. J. Doe,P. J. Doe,G. Doucas,M. R. Dragowsky,M. R. Dragowsky,C. A. Duba,F. A. Duncan,Monica Dunford,J. A. Dunmore,E. D. Earle,E. D. Earle,Steven Elliott,Steven Elliott,Hal Evans,G. T. Ewan,J. Farine,J. Farine,H. Fergani,A. P. Ferraris,R. J. Ford,Joseph A. Formaggio,M. M. Fowler,K. Frame,E.D. Frank,W. Frati,N. Gagnon,J. V. Germani,Salvador Gil,K. Graham,Darren Grant,R. L. Hahn,A. L. Hallin,E. D. Hallman,A. S. Hamer,A. S. Hamer,A. A. Hamian,W. B. Handler,R. U. Haq,C. K. Hargrove,P. J. Harvey,R. Hazama,K. M. Heeger,W. J. Heintzelman,J. Heise,J. Heise,R. L. Helmer,R. L. Helmer,J. D. Hepburn,H. Heron,J. Hewett,Andrew Hime,M. A. Howe,J. G. Hykawy,M. C.P. Isaac,P. Jagam,N. A. Jelley,C. Jillings,G. Jonkmans,G. Jonkmans,K. Kazkaz,P. T. Keener,Joshua R. Klein,A. B. Knox,R. J. Komar,Richard T. Kouzes,T. Kutter,Christopher C. M. Kyba,J. Law,I. T. Lawson,M. Lay,H. W. Lee,K. T. Lesko,J. R. Leslie,I. Levine,W. Locke,S. Luoma,J. Lyon,S. Majerus,H. B. Mak,J. Maneira,J. Manor,A. D. Marino,N. McCauley,N. McCauley,A. B. McDonald,A. B. McDonald,D. S. McDonald,K. McFarlane,G. McGregor,R. Meijer Drees,C. Mifflin,G. G. Miller,G. Milton,B. A. Moffat,M. Moorhead,C. W. Nally,Mark Neubauer,F.M. Newcomer,H. S. Ng,A. J. Noble,A. J. Noble,Eric B. Norman,V. M. Novikov,M. O'Neill,C. E. Okada,R. W. Ollerhead,M. Omori,John L. Orrell,S. M. Oser,A. W. P. Poon,T. J. Radcliffe,A. Roberge,B. C. Robertson,R. G. H. Robertson,R. G. H. Robertson,S. S.E. Rosendahl,J. K. Rowley,V. L. Rusu,E. Saettler,K. K. Schaffer,M. H. Schwendener,Anett Schulke,H. Seifert,H. Seifert,H. Seifert,M. Shatkay,J. J. Simpson,C. J. Sims,David A. Sinclair,David A. Sinclair,P. Skensved,Alan R. Smith,M. W.E. Smith,T. Spreitzer,N. Starinsky,T. D. Steiger,R. G. Stokstad,L. C. Stonehill,R. S. Storey,Bhaskar Sur,Bhaskar Sur,Reda Tafirout,N. Tagg,N. Tagg,N. W. Tanner,R. K. Taplin,M. Thorman,P. M. Thornewell,P. T. Trent,Y. I. Tserkovnyak,R. Van Berg,R. G. Van de Water,R. G. Van de Water,C. J. Virtue,Chris Waltham,J. X. Wang,D. L. Wark,D. L. Wark,D. L. Wark,N. West,J. B. Wilhelmy,J. F. Wilkerson,J. F. Wilkerson,J. R. Wilson,Peter Wittich,J. M. Wouters,Minfang Yeh +205 more
TL;DR: Observations of neutral-current nu interactions on deuterium in the Sudbury Neutrino Observatory are reported, providing strong evidence for solar nu(e) flavor transformation.
Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory
Q. R. Ahmad,R. C. Allen,T. C. Andersen,J. D. Anglin,G. Bühler,J. C. Barton,J. C. Barton,E. W. Beier,M. Bercovitch,J. Bigu,S. D. Biller,R. A. Black,I. Blevis,R. J. Bardman,J. Boger,E. Bonvin,Mark Guy Boulay,M. G. Bowler,T. J. Bowles,S. J. Brice,S. J. Brice,M. C. Browne,T. V. Bullard,T.H. Burritt,T.H. Burritt,K. Cameron,J. Cameron,Yuen-Dat Chan,M. L. Chen,Herbert H. Chen,Xin Chen,Xin Chen,M. C. Chon,B. T. Cleveland,E. T.H. Clifford,E. T.H. Clifford,J. H.M. Cowan,D. F. Cowen,G. A. Cox,Y. Dai,X. Dai,F. Dalnoki-Veress,W. F. Davidson,P. J. Doe,P. J. Doe,P. J. Doe,G. Doucas,M. R. Dragowsky,M. R. Dragowsky,C. A. Duba,F. A. Duncan,J. A. Dunmore,E. D. Earle,E. D. Earle,Steven Elliott,Steven Elliott,Hal Evans,G. T. Ewan,J. Farine,H. Fergani,A. P. Ferraris,R. J. Ford,M. M. Fowler,K. Frame,E.D. Frank,W. Frati,J. V. Germani,J. V. Germani,Salvador Gil,A. Goldschmidt,Darren Grant,R. L. Hahn,A. L. Hallin,E. D. Hallman,A. S. Hamer,A. S. Hamer,A. A. Hamian,R. U. Haq,C. K. Hargrove,P. J. Harvey,R. Hazama,R. Heaton,K. M. Heeger,W. J. Heintzelman,J. Heise,R. L. Helmer,R. L. Helmer,J. D. Hepburn,J. D. Hepburn,H. Heron,J. Hewett,Andrew Hime,M. A. Howe,J. G. Hykawy,M. C.P. Isaac,P. Jagam,N. A. Jelley,C. Jillings,G. Jonkmans,G. Jonkmans,J. Karn,P. T. Keener,Klaus Kirch,Joshua R. Klein,A. B. Knox,R. J. Komar,R. J. Komar,Richard T. Kouzes,T. Kutter,Christopher C. M. Kyba,J. Law,I. T. Lawson,M. Lay,H. W. Lee,K. T. Lesko,J. R. Leslie,I. Levine,W. Locke,M. M. Lowry,S. Luoma,J. Lyon,S. Majerus,H. B. Mak,A. D. Marino,N. McCauley,A. B. McDonald,A. B. McDonald,D. S. McDonald,K. McFarlane,G. McGregor,W. McLatchie,R. Meijer Drees,H. Mes,C. Mifflin,G. G. Miller,G. Milton,B. A. Moffat,M. Moorhead,M. Moorhead,C. W. Nally,Mark Neubauer,F.M. Newcomer,H. S. Ng,A. J. Noble,A. J. Noble,Eric B. Norman,V. M. Novikov,M. O'Neill,C. E. Okada,R. W. Ollerhead,M. Omori,John L. Orrell,S. M. Oser,A. W. P. Poon,T. J. Radcliffe,A. Roberge,B. C. Robertson,R. G. H. Robertson,R. G. H. Robertson,J. K. Rowley,V. L. Rusu,E. Saettler,K. K. Schaffer,A. Schuelke,M. H. Schwendener,H. Seifert,H. Seifert,H. Seifert,M. Shatkay,J. J. Simpson,David A. Sinclair,P. Skensved,Alan R. Smith,M. W.E. Smith,N. Starinsky,T. D. Steiger,R. G. Stokstad,R. S. Storey,Bhaskar Sur,Bhaskar Sur,Reda Tafirout,N. Tagg,N. W. Tanner,R. K. Taplin,M. Thorman,P. M. Thornewell,P. M. Thornewell,P. M. Thornewell,P. T. Trent,P. T. Trent,Y. I. Tserkovnyak,R. Van Berg,R. G. Van de Water,R. G. Van de Water,C. J. Virtue,Chris Waltham,J. X. Wang,D. L. Wark,N. West,J. B. Wilhelmy,J. F. Wilkerson,J. F. Wilkerson,J. R. Wilson,Peter Wittich,J. M. Wouters,Minfang Yeh +205 more
TL;DR: In this paper, the total flux of 8B neutrinos was determined to be (5.44±0.99)×106 cm−2 s−1, in close agreement with the predictions of solar models.
2K
•Journal Article
Sudbury neutrino observatory
J. Boger,R. L. Hahn,J. K. Rowley,A.L. Carter,B. Hollebone,D. Kessler,I. Blevis,F. Dalnoki-Veress,A. Dekok,J. Farine,Darren Grant,C. K. Hargrove,G. Laberge,I. Levine,K. McFarlane,H. Mes,A.T. Noble,V. M. Novikov,M. O'Neill,M. Shatkay,C. Shewchuk,David A. Sinclair,E. T.H. Clifford,R. Deal,E. D. Earle,E. Gaudette,G. Milton,Bhaskar Sur,J. Bigu,J. H.M. Cowan,D.L. Cluff,E. D. Hallman,R. U. Haq,J. Hewett,J. G. Hykawy,G. Jonkmans,R. Michaud,A. Roberge,J. Roberts,E. Saettler,M. H. Schwendener,H. Seifert,D. Sweezey,Reda Tafirout,C. J. Virtue,D.N. Beck,Yuen-Dat Chan,Xin Chen,M. R. Dragowsky,F.W. Dycus,J. Gonzalez,M. C.P. Isaac,Y. Kajiyama,G.W. Koehler,K. T. Lesko,M.C. Moebus,Eric B. Norman,C. E. Okada,A. W. P. Poon,P. Purgalis,A. Schuelke,Alan R. Smith,R. G. Stokstad,S. Turner,I. Zlimen,J.M. Anaya,T. J. Bowles,S. J. Brice,E.I. Esch,Malcolm M. Fowler,A. Goldschmidt,Andrew Hime,A.F. McGirt,G. G. Miller,W.A. Teasdale,J. B. Wilhelmy,J. M. Wouters,J. D. Anglin,M. Bercovitch,W.F. Davidson,R. S. Storey,S. D. Biller,R. A. Black,R. J. Boardman,M. G. Bowler,J. Cameron,B. T. Cleveland,A. P. Ferraris,G. Doucas,H. Heron,C. Howard,N. A. Jelley,A. B. Knox,M. Lay,W. Locke,J. Lyon,S. Majerus,M. Moorhead,M. Omori +98 more
117
Measurement of radium concentration in water with Mn coated beads at the Sudbury Neutrino Observatory
T. C. Andersen,I. Blevis,J. Boger,E. Bonvin,M. L. Chen,B. T. Cleveland,X Dai,F. Dalnoki-Veress,G. Doucas,J. Farine,H. Fergani,A. P. Ferraris,Malcolm M. Fowler,R. L. Hahn,E. D. Hallman,C. K. Hargrove,P. Jagam,N. A. Jelley,A. B. Knox,H.W. Lee,I. Levine,S. Majerus,K. McFarlane,C. Mifflin,Guthrie Miller,A. J. Noble,P. D. Palmer,J. K. Rowley,M. Shatkay,J. J. Simpson,David A. Sinclair,J.-X Wang,J. B. Wilhelmy,Minfang Yeh +33 more
TL;DR: In this article, a method to measure the concentration of and in the heavy water target used to detect solar neutrinos at the Sudbury Neutrino Observatory and in surrounding light water shielding is described.
42
Measurement of 222 Rn dissolved in water at the Sudbury Neutrino Observatory
I. Blevis,J. Boger,E. Bonvin,B. T. Cleveland,X Dai,F. Dalnoki-Veress,G. Doucas,J. Farine,H. Fergani,Darren 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. B. McDonald,K. McFarlane,C. Mifflin,A. J. Noble,S Noël,V. M. Novikov,J. K. Rowley,M. Shatkay,J. J. Simpson,David A. Sinclair,Bhaskar Sur,J.-X Wang,Minfang Yeh,X Zhu +35 more
TL;DR: The technique used at the Sudbury Neutrino Observatory (SNO) to measure the concentration of 222 Rn in water is described in this article, where water from the SNO detector is passed through a vacuum degasser or a membrane contact degasser where dissolved gases, including radon, are liberated.
34